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相关论文: Optical spectral observations of three binary mill…

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We report on multi-band photometric observations of four binary millisecond pulsars with the Gran Telescopio Canarias. The observations led to detection of binary companions to PSRs J1630+3734, J1741+1351 and J2042+0246 in the Sloan g', r'…

We report detection of the binary companion to the millisecond pulsar J2302+4442 based on the deep observations performed with the Gran Telescopio Canarias. The observations revealed an optical source with $r'$ = 23.33$\pm$0.02 and…

太阳与恒星天体物理 · 物理学 2018-08-08 A. Yu. Kirichenko , S. V. Zharikov , D. A. Zyuzin , Yu. A. Shibanov , A. V. Karpova , S. Dai , A. Cabrera-Lavers

We report on photometric and spectroscopic observations of white dwarf companions to four binary radio millisecond pulsars, leading to the discovery of companions to PSRs J0614-3329, J1231-1411 and J2017+0603. We place limits on the…

高能天体物理现象 · 物理学 2015-12-09 C. G. Bassa , J. Antoniadis , F. Camilo , I. Cognard , D. Koester , M. Kramer , S. R. Ransom , B. W. Stappers

Using the SDSS and Pan-STARRS1 survey data, we found a likely companion of the recently discovered binary $\gamma$-ray radio-loud millisecond pulsar J0621+2514. Its visual brightness is about 22 mag. The broad band magnitudes and colours…

太阳与恒星天体物理 · 物理学 2018-07-05 A. V. Karpova , D. A. Zyuzin , Yu. A. Shibanov , A. Yu. Kirichenko , S. V. Zharikov

We report the detection of the likely companion of the binary millisecond pulsar J0740+6620 with the Gran Telescopio Canarias in the $r'$ and $i'$ bands. The position of the detected starlike source coincides with the pulsar coordinates…

太阳与恒星天体物理 · 物理学 2019-03-04 D. M. Beronya , A. V. Karpova , A. Yu. Kirichenko , S. V. Zharikov , D. A. Zyuzin , Yu. A. Shibanov , A. Cabrera-Lavers

We report detection of the binary companion to the millisecond pulsar J1741+1351 with the Gran Telescopio Canarias. The optical source position coincides with the pulsar coordinates and its magnitudes are g' = 24.84(5), r' = 24.38(4) and i'…

太阳与恒星天体物理 · 物理学 2020-01-08 D. A. Zyuzin , A. Yu. Kirichenko , A. V. Karpova , Yu. A. Shibanov , S. V. Zharikov , E. Fonseca , A. Cabrera-Lavers

We report on Keck optical BVRI images and spectroscopy of the companion of the binary millisecond pulsar PSR J0218+4232. A faint bluish (V=24.2, B-V=0.25) counterpart is observed at the pulsar location. Spectra of this counterpart reveal…

天体物理学 · 物理学 2011-05-23 C. G. Bassa , M. H. van Kerkwijk , S. R. Kulkarni

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

We report on spectroscopy of the white-dwarf companion of the millisecond radio pulsar PSR J1012+5307. We find strong Balmer absorption lines, as would be expected for a cool DA white dwarf. The profiles are much narrower than usual,…

天体物理学 · 物理学 2009-10-28 M. H. van Kerkwijk , P. Bergeron , S. R. Kulkarni

The hierarchical triple system PSR J0337+1715 offers an unprecedented laboratory to study secular evolution of interacting systems and to explore the complicated mass-transfer history that forms millisecond pulsars and helium-core white…

We present the identification of the companion star to the intermediate mass binary pulsar J1439-5501 obtained by means of ground-based deep images in the B, V and I bands, acquired with FORS2 mounted at the ESO-VLT. The companion is a…

太阳与恒星天体物理 · 物理学 2015-06-16 C. Pallanca , B. Lanzoni , E. Dalessandro , F. R. Ferraro , A. Possenti , M. Salaris , M. Burgay , -

We present the discovery of a binary millisecond pulsar (MSP), PSR J2322$-$2650, found in the Southern section of the High Time Resolution Universe survey. This system contains a 3.5-ms pulsar with a $\sim10^{-3}$ M$_{\odot}$ companion in a…

We analyse archival optical data on the binary companion to the millisecond pulsar \j1045\ obtained with the Very Large Telescope. A possible optical counterpart candidate %source position coincides with the pulsar coordinates is found at…

太阳与恒星天体物理 · 物理学 2023-07-11 A. V. Bobakov , D. A. Zyuzin , Yu. A. Shibanov

We report identification of the optical counterpart to the companion of the millisecond pulsar J2317+1439. At the timing position of the pulsar, we find an object with $g=22.96\pm0.05$, $r=22.86\pm0.04$ and $i=22.82\pm0.05$. The magnitudes…

太阳与恒星天体物理 · 物理学 2017-06-28 S. Dai , M. C. Smith , S. Wang , S. Okamoto , R. X. Xu , Y. L. Yue , J. F. Liu

Optical observations of the companions of pulsars can help determine the properties of the binaries, as well as those of their components, and give clues to the preceding evolution. In this review, we first describe the different classes of…

天体物理学 · 物理学 2007-05-23 M. H. van Kerkwijk , C. G. Bassa , B. A. Jacoby , P. G. Jonker

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 present the discovery of the variable optical counterpart to PSR J2055+1545, a redback millisecond pulsar, and the first radial velocity curve of its companion star. The multi-band optical light curves of this system show a $0.4$$-$$0.6…

We analyse 55 ks of Chandra X-ray observations of the Galactic globular cluster M13. Using the latest radio timing positions of six known millisecond pulsars (MSPs) in M13 from Wang et al. (2020), we detect confident X-ray counterparts to…

高能天体物理现象 · 物理学 2021-01-27 Jiaqi Zhao , Yue Zhao , Craig O. Heinke

Previous optical and radio observations of the binary millisecond pulsar PSR J1640+2224 have come to inconsistent conclusions about the identity of its companion, with some observations suggesting the companion is a low-mass helium-core…

太阳与恒星天体物理 · 物理学 2018-03-20 Sarah J. Vigeland , Adam T. Deller , David L. Kaplan , Alina G. Istrate , Benjamin W. Stappers , Thomas M. Tauris

Milli-second pulsars (MSPs) are rapidly spinning neutron stars, with spin periods P_s <= 10 ms, which have been most likely spun up after a phase of matter accretion from a companion star. In this work we present the results of the search…

高能天体物理现象 · 物理学 2015-09-30 V. Testa , R. P. Mignani , C. Pallanca , A. Corongiu , F. R. Ferraro
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