Kyr psr. Work horses Current (secure) member list Zoom-in on some recent 'new' members AX J1838.0-0655, PSR J2229+6114 and IGR J18490-0000 Population comparisons Summary & conclusions "The fast and furious", ESAC-Workshop, Madrid, 22-24th May 2013 2 High-energy g-ray (>100 MeV) pulsar population Sample used in this work: # 101 from ...

A similar upward evolution is seen for PSR J1734-3333, which has a measured n of 0.9±0.2 (Espinoza et al. 2011b) and is speculated to attain the rotational properties of a magnetar in ∼ 30 kyr ...

Kyr psr. The pulsar's spin-down rate implies a rotation-powered luminosity E-dot = 1.2x10{sup 38} erg s{sup -1}, a surface dipole magnetic field strength B{sub s} = 1.0 x 10{sup 12} G, and a characteristic age of 8.9 kyr. PSR J2022+3842 is thus the second-most energetic Galactic pulsar known, after the Crab pulsar, as well as the most rapidly …

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PSR J2022+3842 is a young, energetic pulsar with a characteristic age of 8.9 kyr and spin down power 3.0 x 10 37 erg s -1 . Located in supernova remnant G76.9+1.0, and spatially coincident with a Fermi LAT source, pulsations with a period of ~48.6 ms have been reported in radio by the GBT, as well in the X-ray band by Chandra, RXTE, and XMM-Newton.The pulsar's spin-down rate implies a rotation-powered luminosity E-dot = 1.2x10{sup 38} erg s{sup -1}, a surface dipole magnetic field strength B{sub s} = 1.0 x 10{sup 12} G, and a characteristic age of 8.9 kyr. PSR J2022+3842 is thus the second-most energetic Galactic pulsar known, after the Crab pulsar, as well as the most rapidly rotating ...

and GeV γ-ray bands. W44 hosts the pulsar PSR B1853+01, a 20 kyr pulsar with dE/dt= 4.3 x 10e35 erg s-1 located approx. 3 kpc away. W44 has not been detected by H.E.S.S. during the HGPS, but H.E.S.S. reported significant emission with only one of their analysis chains at the location of W44, without claiming a detection (Abdalla et al., 2018)."This and other considerations lead us to conclude that the pulsar is possibly older than 45 − 100 kyr. PSR J1734−3333 is a pulsar with rotational properties that place it between standard ...Bs = 1.0×1012 G, and a characteristic age of 8.9 kyr. PSR J2022+3842 is thus the second-most ener-getic Galactic pulsar known, after the Crab, as well as the most rapidly-rotating young, radio-bright pulsar known. The radio pulsations are highly dispersed and broadened by interstellar scattering, andWhile 3/4 inch metal pipe or thick wall conduit, make a strong closet rod that won't sag, it's not very attractive to look at. To improve the looks, cut a piece of 1 inch diameter ...The pulsar's spin-down rate implies a rotation-powered luminosity E = 1.2 X 10(exp 38) erg/s, a surface dipole magnetic field strength B(sub S), = 1.0 X 10(exp 12) G, and a characteristic age of 8.9 kyr. PSR J2022+3842 is thus the second-most energetic Galactic pulsar known, after the Crab, as well as the most rapidly-rotating young, radio ...The survey has so far resulted in the discovery of 15 radio pulsars, including a pulsar with a characteristic age of ∼18 kyr, PSR J2004+3429, and a highly eccentric, binary millisecond pulsar ...We have obtained a deep 670 ks CXO ACIS image of the remarkable pulsar wind nebula (PWN) of PSR J1709-4429, in 4 epochs during 2018-2019. Comparison with an archival 2004 data set provides a pulsar proper motion mu = 13 \\pm 3 mas/yr at a PA of 86 \\pm 9 degree (1 sigma combined statistical and systematic uncertainties), precluding birth near the center of SNR G343.1-2.3. At the pulsar's ...We report the discovery of three radio pulsars (PSR J0631+10, J 1843+20, and J 1908+0457) in a search targeted at Einstein IPC X-ray sources. The fastest, J0631+10, has a period of 0.288 s and high period derivative (Pdot = 104 x 10 -15 s s -1 ) corresponding to a spin-down age of only 43 kyr. From 1400 MHz to 2380 MHz the radio spectrum is nearly flat, and the pulse profile is very ...

We report the discovery of PSR J2022+3842, a 24 ms radio and X-ray pulsar in the supernova remnant G76.9+1.0, in observations with the Chandra X-ray telescope, the Robert C. Byrd Green ... and a characteristic age of 8.9 kyr. PSR J2022+3842 is thus the second-most ener-getic Galactic pulsar known, after the Crab, as well as the most rapidly ...PSR J1446-4701 turned out to be a non-eclipser with possibly low (face-on) orbital inclination, with emission from both the pulsar and the intra-binary shock observable throughout the binary orbit. PSR J1311-3430 is a known eclipser, in which hints of spectral variability have been found, between pulsar superior and inferior conjunction phases.Timing observations of PSR J2021+3651 revealed that al-though it is dim, it is young and energetic (characteristic age c P=2P˙ ¼ 17 kyr and spin-down energy E˙ 4 2IP˙=P3 ¼ 3:6 ;1036 ergs s 1, assuming a moment of inertia I ¼ 1045 g cm2) and a likely counterpart to the ASCA X-ray source AX J2021.1+3651 and the EGRET -ray source GeV J2020 ...

PSR J1906+0722 is a young, energetic, isolated pulsar, with a spin frequency of 8.9 Hz, a characteristic age of 49 kyr, and spin-down power 1.0× {10} 36 erg s-1. In 2009 August it suffered one of the largest glitches detected from a gamma-ray pulsar ({{Δ }}f/f≈ 4.5× {10}-6). Remaining undetected in dedicated radio follow-up observations ...

Abstract. We present the discovery and timing of the young (age ∼28.6 kyr) pulsar PSR J0837–2454. Based on its high latitude ( b = 98) and dispersion measure (DM = 143 pc cm −3 ), the pulsar appears to be at a z -height of >1 kpc above the Galactic plane, but near the edge of our Galaxy.

Paleoclimate time series and the 100-kyr band variability associated with each record. (a) Magnetic susceptibility (MS) stack record of Sun et al. from the Chinese Loess Plateau (MS of Chinese loess sediments is a widely used EASM intensity proxy [An et al., 2001]). (b) Benthic δ 18 O record from ODP Site 659 (blue) and benthic δ 18 O stack record synthesized by Lisiecki and Raymo (red).Robert Kyr poses in St. Martin's Lutheran Church in Austin, Texas. Kyr, the composer-in-residence for the concert series "Renaissance and Response", created original music for the concerts.The 405-kyr cycles in proxy records for the East Asian summer monsoon and global ice volume intensified and became phase-locked to eccentricity forcing at ~ 4.5 Ma.We revised previous forcing mechanism hypothesis for Pliocene intensification of the 405-kyr cycles in paleoclimatic records and proposed that the establishment of salinity difference between the Pacific Ocean and the Caribbean Sea ...Aug 18, 2023 · The angular separation between PSR J2021+3651 and the centroid of eHWC J2019+368 is . If PSR J2021+3651 was born near the centroid of eHWC J2019+368 and traveled to the current location at a constant speed, the corresponding transverse velocity of the pulsar is km s −1, where t 16 is the true age scaled to 16 kyr.Velkeer, Velky Kyr. 2,289 likes · 123 talking about this · 296 were here. VELKEER winery and vineyards - Nitra region - Slovakia

The asset protection allowance was eliminated on the latest FAFSA form. Here's what it means for families applying for college financial aid. By clicking "TRY IT", I agree to recei...We report on the X-ray emission properties of the pulsar PSR J1849$-$0001 and its wind nebula (PWN), as measured by Chandra, XMM-Newton, NICER, Swift, and NuSTAR. In the X-ray data, we detected the 38-ms pulsations of the pulsar up to $\\sim$60 keV with high significance. Additionally, we found that the pulsar's on-pulse spectral energy distribution displays significant curvature, peaking at ...Observations by the High-Altitude Water Cherenkov Observatory (HAWC) and Milagro have detected spatially extended TeV sources surrounding middle-aged (t ∼ 100-400 kyr) pulsars like Geminga and PSR B0656+14, which have been named "TeV halos," representing very extended TeV pulsar wind nebulae (PWNe) powered by relatively old pulsars. A few more HAWC-detected sources have been suggested to be ...ages to two characteristic features in the o record: 11.5 kyr for the end of the Younger Dryas event 1-12 and 110 kyr for the marine isotope stage (MIS) 5d4, which appear at depths of 1,624The timing solution, reported by Levin et al. , implies a very high surface magnetic field of 2.8 1 G and a characteristic age of 4 kyr. PSR J1622-4950 has a flat radio spectrum and a highly variable flux density and pulse profile [8-10, 16, 89], which is similar to other radio magnetars.Apr 19, 1996 · We present radio observations of a region in the vicinity of the young pulsar PSR B1853+01 in the supernova remnant W44. The pulsar is located at the apex of an extended feature with cometary morphology. We argue on the basis of its morphology and its spectral index and polarization properties that this is a synchrotron nebula produced by the spin-down energy of the pulsar. The geometry and ...PSR J2022+3842 was discovered in SNR G76.9+1.0 as an energetic rotation-powered young pulsar and has period of 48 ms (Arzoumanian et al. 2011, Arumugasamy et al. 2014). It is a Vela-like pulsar due to its spin down energy rate of 3.0 1037 erg/s and the characteristic age of 8.9 kyr. Though radio and X-ray pulse emission were observed, the ...The survey has so far resulted in the discovery of 15 radio pulsars, including a pulsar with a characteristic age of ∼18 kyr, PSR J2004+3429, and a highly eccentric, binary millisecond pulsar, PSR J1946+3417.KYR Music offers new equipment to buy and a variety of services like rental service, music lessons, and instrument repairs. The store, located at 14560 Pipeline Ave., is open from noon to 8 p.m. Monday through Friday, and 10 a.m. to 3 p.m. Saturdays. Information: 597-0750 and www.kyrmusic.com.We present radio observations of a region in the vicinity of the young pulsar PSR B1853+01 in the supernova remnant W44. The pulsar is located at the apex of an extended feature with cometary morphology. We argue on the basis of its morphology and its spectral index and polarization properties that this is a synchrotron nebula produced by the spin-down energy of the pulsar. The geometry and ...The characteristic age of PSR J1734−3333 estimated from its current spin down rate implies that it is a young pulsar (τ c = 8.1 kyr). However, the time derivative of its spin-down rate differs markedly from that assumed for normal radio pulsars, meaning its actual age is uncertain.PSR J1048-5832 is a Vela-like (P=123.6 ms; tau~20.3 kyr) gamma-ray pulsar detected by Fermi, at a distance of ~2.7 kpc and with a rotational energy loss rate dot{E}_{SD} ~2 x 10^{36} erg/s. The PSR J1048-5832 field has been observed with the VLT in the V and R bands. We used these data to determine the colour of the object detected …Particularly interesting is the association of the pulsar PSR J0538+2817 with the young supernova remnant S147 and an age of only 30±4 kyr (Kramer et al. 2003; Dinçel et al. 2015), because the ...PWNe with ages up to several kyr. Recent X-ray observations have shown the presence 1 SchoolofCosmicPhysics ... Uchiyama et al. (2009) found a largely extended nebula from PSR B1823-13 as-sociated with HESS J1825−137, which could not be detected with Chandra (Pavlov et al. 2008) or XMM-Newton(Gaensler et al. 2003) observations. ...gamma-ray source around the location of the middle-aged (207.8 kyr) pulsar PSR J0622+3749 with the Large High Altitude Air Shower Observatory (LHAASO). - The source is detected with a significance of 8.2σ for E > 25 TeV assuming a Gaussian template." Source Position: From Aharonian et al. (2021):Specialties: Top rated in Chino We Specialize in: - Musical Instrument Lessons - Musical Instrument Rental - Musical Instruments - Music Instruction-Instrumental - Musical Instruments-Repair - Music Sheet - Music Stores Established in 2002. KYR is the realization of a dream of Karen and Richard. Richard started playing at age 10, like many of today's kids, and understands the need of a strong ...PSR B0740-28 has a spin-frequency of 6 Hz and a characteristic (spin-down) age of 160 kyr. We monitor PSR B0740-28 for 1 hour per day with the 42-ft telescope and approximately weekly with the Lovell telescope.This and other considerations lead us to conclude that the pulsar is possibly older than 45 − 100 kyr. PSR J1734−3333 is a pulsar with rotational properties that place it between standard ...

According to Thorsett et al. (2003), the age of the Monogem Ring from Sedov modeling is 86 kyr, which is consistent with 110 kyr, the characteristic spindown age of PSR B0656+14. They also showed ...We report the discovery of an extended very-high-energy (VHE) gamma-ray source around the location of the middle-aged (207.8 kyr) pulsar PSR J 0622 +3749 with the Large High-Altitude Air Shower Observatory (LHAASO). The source is detected with a significance of 8.2 σ for E >25 TeV assuming a Gaussian template. The best-fit location is (right ascension, declination) =(95.47 ° ±0.11 ° ,37 ...We report the discovery of PSR J2022+3842, a 24 ms radio and X-ray pulsar in the supernova remnant G76.9+1.0, in observations with the Chandra X-ray telescope, the Robert C. Byrd Green Bank Radio Telescope, and the Rossi X-ray Timing Explorer (RXTE). The pulsar's spin-down rate implies a rotation-powered luminosity Edot = 1.2 x 10^{38} erg/s, a surface dipole magnetic field strength B_s = 1.0 ...We present radio observations of a region in the vicinity of the young pulsar PSR B1853+01 in the supernova remnant W44. The pulsar is located at the apex of an extended feature with cometary morphology. We argue on the basis of its morphology and its spectral index and polarization properties that this is a synchrotron nebula produced by the spin-down energy of the pulsar. The geometry and ...PSR J1747-2958 is a young (tau=26 kyr), energetic (Edot=2.5x10^36 erg/s) supersonic pulsar at an estimated distance d=5 kpc. It powers the Mouse pulsar wind nebula (PWN; G359.23-.82), which ...Observations by the High-Altitude Water Cherenkov Observatory (HAWC) and Milagro have detected spatially extended TeV sources surrounding middle-aged (t ∼ 100-400 kyr) pulsars like Geminga and PSR B0656+14, which have been named "TeV halos," representing very extended TeV pulsar wind nebulae (PWNe) powered by relatively old …Ruthless and cold, Kyr climbed to the top rank of the League High Command by killing anyone who stood in his way. Out of all the assassins sent after Nykyrian, he was the only one who survived. Something he hasn't forgotten since that encounter cost him his right eye. He's never been happy about the fact that the League pardoned Nykyrian.HESS J1825-137 is one of the most powerful and luminous TeV gamma-ray pulsar wind nebulae (PWNe), making it an excellent laboratory to study particle transportation around pulsars. We present a model of the (diffusive and advective) transport and radiative losses of electrons from the pulsar PSRJ1826-1334 powering HESSJ1825-137 using interstellar medium gas (ISM) data, soft photon fields and a ...

PSR J2032+4127 is co-located with the extended TeV gamma-ray source, TeV J2032+4130, and may be physically associated with it. Source Information: From VERITAS and MAGIC Collaborations (2018): - "We report on observations of the pulsar / Be star binary system. PSR J2032+4127 / MT91 213 in the energy range between 100 GeV and 20 TeV.- "PSR J1809-1917 is a young (age = 51 kyr) energetic (E-dot = 1.8 x10e36 erg s−1 ) radio pulsar powering a pulsar wind nebula (PWN). We report on the results of three Chandra X-ray Observatory observations which show that the PWN consists of a small (approx. 20'') bright compact nebula (CN) and faint extended emission seen up to 20 from the ...The pulsar's spin-down rate implies a rotation-powered luminosity E-dot = 1.2x10{sup 38} erg s{sup -1}, a surface dipole magnetic field strength B{sub s} = 1.0 x 10{sup 12} G, and a characteristic age of 8.9 kyr. PSR J2022+3842 is thus the second-most energetic Galactic pulsar known, after the Crab pulsar, as well as the most rapidly rotating ...This and other considerations lead us to conclude that the pulsar is possibly older than 45 − 100 kyr. PSR J1734−3333 is a pulsar with rotational properties that place it between standard ...Title: Study of a pulsar wind nebula candidate around the intermediate-age pulsar PSR J1413-6205 with H.E.S.S. ... {35}$ to $10^{37}$ erg s$^{-1}$ for ages between 13.6 and 62.8 kyr. Extended emission is detected with H.E.S.S. (High Energy Stereoscopic System) in their vicinity, notably around the pulsar PSR J1413-6205.We report on the setup and initial discoveries of the Northern High Time Resolution Universe survey for pulsars and fast transients, the first major pulsar survey conducted with the 100-m Effelsberg radio telescope and the first in 20 years to observe the whole northern sky at high radio frequencies. Using a newly developed 7-beam receiver system combined with a state-of-the-art polyphase ...Prayer Times Today. Prayer Times Today in Franconville, Île-de-France France are Fajar Prayer Time 04:33 AM, Dhuhur Prayer Time 01:48 PM, Asr Prayer Time 05:59 PM, Maghrib Prayer Time 09:33 PM & Isha Prayer Time 11:02 PM. Get the most accurate Franconville Azan and Namaz times with both; weekly Salat timings and monthly Salah timetable.Aug 1, 2014 · The U.S. Department of Energy's Office of Scientific and Technical Information1. Introduction [2] All serious students of Earth's climate history have heard of the "100 kyr problem" of Milankovitch orbital theory, namely the lack of an obvious explanation of the dominant ∼100 kyr periodicity in climate records of the last 800,000 years. However, few have considered an equally perplexing characteristic of Earth's climate, one that similarly defies simple physical ...In comparison to τ c , the 10-30 kyr age estimated for MSH 11-61A suggests that the pulsar was born in the SNR with initial period in the range 54 <= P 0 <= 60 ms. PSR J1101-6101 is the least energetic of the 15 rotation-powered pulsars detected by INTEGRAL, and has a high efficiency of hard X-ray radiation and jet power.There have been a thousand or more articles written about how to have a successful long-term relationship or m There have been a thousand or more articles written about how to have...Download scientific diagram | — X-ray images of the old PWNe above 2 keV in Galactic coordinates. The rectangles represent the region for the size estimation. The "+" and "X" marks are ...Abstract. We present the discovery and timing of the young (age ∼28.6 kyr) pulsar PSR J0837–2454. Based on its high latitude ( b = 98) and dispersion measure (DM = 143 pc cm −3 ), the pulsar appears to be at a z -height of >1 kpc above the Galactic plane, but near the edge of our Galaxy.SNR ∼1-7 kyr). PSR J1844−0256 was discovered in a search of AXP AX J1845−0258. Its P = 273 ms and DM = 820 pc cm−3 with a large scattering tail (τ scat ∼40 ms). The period derivative obtained from observations taken a year apart indicates that the pulsar is much older (τ c ∼300 kyr) than the target AXP (τ AXP ∼<10PSR J1357−6429 is a young (characteristic age 7.3 kyr) and energetic (spin-down luminosityĖ = 3.1×10 36 ergs s −1 ) radio pulsar with a period of 166 ms (Camilo et al. 2004).The nine pulsars have spin frequencies between 3 and 12 Hz, and characteristic ages ranging from 17 kyr to 3 Myr. Two of them, PSRs J1803-2149 and J2111+ 4606, are …Download Table | Observed parameters of the SNRs confirmed by these observations from publication: Confirmation of New Supernova Remnants near the Galactic Centre | We have made deep observations ...The 173-kyr band obliquity signals are correlated well with orbital solution in the eolian red clay for the first time, although it is not the first time we have seen in the eastern CLP (Figures 4b, 5c, and 5d; Anwar et al., 2015). Therefore, through the new astronomical solution, we can see both the 173 kyr obliquity and the 405 kyr ...

PSR B1849+00 has a spin-down power of ∼4 × 10 32 erg s −1 and a surface magnetic field of ∼3 × 10 13 G (see Hobbs et al. 2004), located 8.4 ± 1.7 kpc from us (Cordes & Lazio 2003). To examine their relative contribution of γ -rays, we conservatively assume for each of them a shorter distance d = 7 kpc from us and a narrower beam solid ...

The velocity and characteristic age of PSR J1825-1446 make it incompatible with SNR G016.8-01.1. There are no clear OB associations or SNRs crossing the past trajectory of PSR J1825-1446. We estimate the age of the pulsar to be 80-245 kyr, which is compatible with its characteristic age.

The survey has so far resulted in the discovery of 15 radio pulsars, including a pulsar with a characteristic age of ∼18 kyr, PSR J2004+3429, and a highly eccentric, binary millisecond pulsar ...The X-ray spectrum of PSR J1852+0040 is best characterized by a blackbody model of temperature kT BB =0.44+/-0.03 keV, radius R BB ~0.9 km, and L bol =3.7×10 33 ergs s -1 at d=7.1 kpc. ... 3×10 12 G, and the spin-down age is τ>24 kyr. The latter exceeds the remnant's estimated age, suggesting that the pulsar was born spinning near its ...PSR J1048-5832 is a Vela-like (P=123.6 ms; tau~20.3 kyr) gamma-ray pulsar detected by Fermi, at a distance of ~2.7 kpc and with a rotational energy loss rate dot{E}_{SD} ~2 x 10^{36} erg/s. The PSR J1048-5832 field has been observed with the VLT in the V and R bands. We used these data to determine the colour of the object detected closest to the Chandra position (Star D) and confirm that it ...3.1 PSR B0154+61 (J0157+6212, τ=200 kyr) Although data on PSR B0154+61 have been collected at Jodrell Bank for more than 10 yr since MJD 46866, this pulsar suffered its first observed glitch near MJD 48504. The glitch was quite small with the size of the frequency jump equal to 2.46 × 10 −9.In this study, we have carried out paleointensity experiments on 918 specimens spanning the last ∼7 kyr, including pottery fragments, baked clay and slag, collected from Shandong, Liaoning, Zhejiang and Hebei Provinces in China. Approximately half of the specimens yielded results that passed strict data selection criteria and give high-fidelity paleointensities.We report on the setup and initial discoveries of the Northern High Time Resolution Universe survey for pulsars and fast transients, the first major pulsar survey conducted with the 100-m Effelsberg radio telescope and the first in 20 years to observe the whole northern sky at high radio frequencies. Using a newly developed 7-beam receiver system combined with a state-of-the-art polyphase ...Novatek News: This is the News-site for the company Novatek on Markets Insider Indices Commodities Currencies Stocks

ardha shdn znsks ba dkhtran bakrhsks synmatake me to kohl Kyr psr skys dagh [email protected] & Mobile Support 1-888-750-4139 Domestic Sales 1-800-221-7891 International Sales 1-800-241-2666 Packages 1-800-800-6143 Representatives 1-800-323-5784 Assistance 1-404-209-2599. We discuss PSR J1740 + 1000, one of five pulsars recently discovered in a search of 470 deg at 430 MHz during the upgrade of the 305 m Arecibo Telescope. The period P = 154 ms and period derivative P = 2.1 x 10(exp -14) s s(exp -1) imply a spin-down age tau(sub s) = P/2P = 114 kyr that is smaller than 95% of all known pulsars.. sksy awyzwn This and other considerations lead us to conclude that the pulsar is possibly older than 45 − 100 kyr. PSR J1734−3333 is a pulsar with rotational properties that place it between standard ...In comparison to τ c , the 10-30 kyr age estimated for MSH 11-61A suggests that the pulsar was born in the SNR with initial period in the range 54 <= P 0 <= 60 ms. PSR J1101-6101 is the least energetic of the 15 rotation-powered pulsars detected by INTEGRAL, and has a high efficiency of hard X-ray radiation and jet power. new orleans obituary timespicayunesasha carl weber The pulsar's spin-down rate implies a rotation-powered luminosity erg s−1, a surface dipole magnetic field strength Bs = 1.0 × 1012 G, and a characteristic age of 8.9 kyr. PSR J2022+3842 is thus the second-most energetic Galactic pulsar known, after the Crab pulsar, as well as the most rapidly rotating young, radio-bright pulsar known. fylm sksyhdaflam sks trky qdym New Customers Can Take an Extra 30% off. There are a wide variety of options. Know Your Rights when interacting with immigration and the police.The links addressed in this presentation are below:USCIS Website - www.uscis.gov· I...PSR J0537−6910 is a young, energetic, rotation-powered X-ray pulsar with a spin period of 16 ms located in the Large Magellanic Cloud. We have searched for previously undetected radio pulsations (both giant and standard) from this pulsar in ... c < 10 kyr), energetic pulsars (of which the Crab pulsar is the prototype) that are known. No radio pulsations …PSR J1928 + 1746, a 69-ms pulsar with a characteristic age of 82 kyr, is a plausible candidate for association with the unidentified EGRET source 3EG J1928 + 1733. PSR J1906 + 0746 is a 144-ms, non-recycled pulsar in a relativistic binary with an orbital period of 3.98 hr. The rate of periastron advance implies a total system mass of 2.4 M ...