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相关论文: A Binary Millisecond Pulsar in Globular Cluster NG…

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We report the discovery of seven new millisecond pulsars during 20 cm searches of 19 globular clusters using the recently upgraded Arecibo Telescope and the new Green Bank Telescope (GBT). Five of the pulsars are in compact binaries, three…

We present 98 spectroscopic binary orbits resulting from our ongoing radial-velocity survey of the old (7 Gyr) open cluster NGC 188. All but 13 are high-probability cluster members based on both radial-velocity and proper-motion membership…

太阳与恒星天体物理 · 物理学 2015-12-17 Aaron M. Geller , Robert D. Mathieu , Hugh C. Harris , Robert D. McClure

We describe the status of a project whose main goal is to detect variability along the extreme horizontal branch of the globular cluster NGC 6752. Based on Magellan 6.5m data, preliminary light curves are presented for some candidate…

We present an evolutionary scenario for the spin-up and evolution of binary millisecond pulsars, according to which the companion of the pulsar PSR J 1740-5340, recently discovered as a binary with orbital period of 32.5 hr in the Globular…

天体物理学 · 物理学 2009-11-07 Luciano Burderi , Francesca D'Antona , Marta Burgay

We present observations of fields containing eight recently discovered binary millisecond pulsars using the telescopes at MDM Observatory. Optical counterparts to four of these systems are detected, one of which, PSR J2214+3000, is a novel…

高能天体物理现象 · 物理学 2015-06-18 Joshua Schroeder , Jules Halpern

PSRJ1910-5959A (J1910A) is a binary millisecond pulsar in a 0.837 day circular orbit around a helium white dwarf (HeWD) companion. This pulsar is located 6.3 arcmin away from the centre of the globular cluster NGC6752. Given the large…

We report the discovery of PSR J1906+0746, a young 144-ms pulsar in a highly relativistic 3.98-hr orbit with an eccentricity of 0.085 and expected gravitational wave coalescence time of 300 Myr. The new pulsar was found during precursor…

We report on the discovery and analysis of an X-ray pulsar, AX J0058-7203, in the Small Magellanic Cloud. This pulsar exhibits coherent pulsations at P= 280.3 s with a double-peak structure. The X-ray spectrum is well fitted with a simple…

天体物理学 · 物理学 2015-06-24 Masahiro Tsujimoto , Kensuke Imanishi , Jun Yokogawa , Katsuji Koyama

We report the discovery of 13 new pulsars in the globular cluster NGC 1851 by the TRAPUM Large Survey Project using the MeerKAT radio telescope. The discoveries consist of six isolated millisecond pulsars (MSPs) and seven binary pulsars, of…

Based on 24h high speed photometry of the hybrid PG 1159 star Abell 43, we have detected 6 sighificant pulsations with periods between 2380 s and 6075 s. A short (4h) run on the almost spectroscopic twin NGC 7094 central star resulted in…

天体物理学 · 物理学 2009-11-13 J. -E. Solheim , G. Vauclair , A. S. Mukadam , R. Janulis , V. Dobrovolskas

We report the discovery of an eclipsing X-ray binary with a 3.62-hr period within 24" of the center of the dwarf starburst galaxy NGC 4214. The orbital period places interesting constraints on the nature of the binary, and allows for a few…

(abridged) PSR J1903+0327, a millisecond pulsar in an eccentric (e = 0.44) 95-day orbit with a (~ 1Msun) companion poses a challenge to our understanding of stellar evolution in binary and multiple-star systems. Here we describe optical and…

We observed the nearby, low-density globular cluster M71 (NGC 6838) with the Chandra X-ray Observatory to study its faint X-ray populations. Five X-ray sources were found inside the cluster core radius, including the known eclipsing binary…

We have used deep high-resolution multiband images taken at the ESO Very Large Telescope to identify the optical binary companion to the millisecond pulsar (PSR J1911-5958A) located in the halo of the Galactic Globular Cluster NGC6752. The…

天体物理学 · 物理学 2009-11-10 Francesco R. Ferraro , Andrea Possenti , Elena Sabbi , Nichi D'Amico

This study continues our investigation of early-type binaries using high-precision broad-band polarimetry, focusing on HD 165052, a massive O+O-type binary in the young cluster NGC 6530. Our aim was to monitor linear polarization variations…

太阳与恒星天体物理 · 物理学 2025-05-21 Yasir Abdul Qadir , Andrei V. Berdyugin , Vilppu Piirola , Takeshi Sakanoi , Masato Kagitani , S. V. Berdyugina

We present a general method for determining the masses and orbital parameters of binary millisecond pulsars with long orbital periods (P_orb >> 1 yr), using timing data in the form of pulse frequency derivatives. We apply our method to…

天体物理学 · 物理学 2009-10-28 K. J. Joshi , F. A. Rasio

A search for pulsations from the Be X-ray binary SAX J2239.3+6116, through observations with the Narrow Field Instruments on BeppoSAX and the Proportional Counter Array on RXTE, yielded the clear presence of a 1247 s coherent oscillation.…

天体物理学 · 物理学 2009-11-07 J. J. M. in 't Zand , J. Swank , R. H. D. Corbet , C. B. Markwardt

We report on the discovery of the companion star to the millisecond pulsar J1342+2822B in the globular cluster M3. We exploited a combination of near-ultraviolet and optical observations acquired with the Hubble Space Telescope in order to…

高能天体物理现象 · 物理学 2019-04-17 M. Cadelano , F. R. Ferraro , A. G. Istrate , C. Pallanca , B. Lanzoni , P. C. C. Freire

We report the discovery of two new millisecond pulsars (PSRs J0024$-$7204aa and J0024$-$7204ab) in the globular cluster 47\,Tucanae (NGC 104). Our results bring the total number of pulsars in 47\,Tucanae to 25. These pulsars were discovered…

高能天体物理现象 · 物理学 2016-03-23 Zhichen Pan , George Hobbs , Di Li , Alessandro Ridolfi , Pei Wang , Paulo Freire

The low mass X-ray binary (LMXB) IGR J17480-2446 in the globular cluster Terzan 5 harbors an 11 Hz accreting pulsar. This is the first object discovered in a globular cluster with a pulsar spinning at such low rate. The accreting pulsar is…

高能天体物理现象 · 物理学 2015-06-03 A. Patruno , M. A. Alpar , M. van der Klis , E. P. J. van den Heuvel
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