中文
相关论文

相关论文: 2S1553-542: a Be/X-ray binary pulsar on the far si…

200 篇论文

High mass X-ray binaries hosting red supergiant (RSG) donors are a rare but crucial phase in massive stellar evolution, with only one source previously known in the Milky Way. In this letter, we present the identification of the second…

太阳与恒星天体物理 · 物理学 2023-09-15 Kishalay De , Fiona A. Daly , Roberto Soria

We present the results of optical observations performed between May and September 1998 of the stars within the position error circle of the recently discovered 12min pulsating X-ray source 1WGA J1958.2+3232. Based on photometry and…

天体物理学 · 物理学 2007-05-23 G. L. Israel , S. Covino , V. F. Polcaro , L. Stella

SWIFT J1626.6-5156 is an X-ray pulsar that was discovered in December 2005 during an X-ray outburst. Although the X-ray data suggest that the system is a high-mass X-ray binary, very little information exists on the nature of the optical…

高能天体物理现象 · 物理学 2015-05-28 P. Reig , E. Nespoli , J. Fabregat , R. Mennickent

Two faint X-ray pulsars, AX J1749.2-2725 and AX J1749.1-2733, located in the direction to the Galactic Center, were studied in detail using data of INTEGRAL, XMM-Newton and Chandra observatories in X-rays, the SOFI/NTT instrument in…

高能天体物理现象 · 物理学 2015-05-19 D. Karasev , A. Lutovinov , R. Burenin

We present results of a detailed investigation of the poorly studied X-ray pulsar XTE J1858+034 based on the data obtained with the NuSTAR observatory during the outburst of the source in 2019. The spectral analysis resulted in the…

We present a detailed NIR/optical/UV study of the transient low mass X-ray binary 1RXS J180408.9-342058 performed during its 2015 outburst, aimed at determining the nature of its companion star. We obtained three optical spectra at the 2.1…

太阳与恒星天体物理 · 物理学 2016-03-02 M. C. Baglio , P. D'Avanzo , S. Campana , P. Goldoni , N. Masetti , T. Munoz-Darias , V. Patino-Alvarez , V. Chavushyan

We report on analysis of properties of the X-ray binary pulsar GROJ1750-27 based on X-ray (Chandra, Swift, and Fermi/GBM), and near-infrared (VVV and UKIDSS surveys) observations. An accurate position of the source is determined for the…

高能天体物理现象 · 物理学 2019-02-20 A. Lutovinov , S. Tsygankov , D. Karasev , S. Molkov , V. Doroshenko

Low-mass X-ray binaries are binary systems composed of a compact object and a low-mass star. Recently, a new class of these systems, known as symbiotic $X$-ray binaries (with a neutron star with a M-type giant companion), has been…

天体物理学 · 物理学 2009-11-13 A. A. Nucita , S. Carpano , M. Guainazzi

We report the discovery with BeppoSAX of a new 170.84 +/- 0.04 s X-ray pulsar, 1SAX J1324.4-6200, found serendipitously in the field of the X-ray binary X1323-619 in 1997 August. The source and periodicity are also detected in archival ASCA…

天体物理学 · 物理学 2007-05-23 L. Angelini , M. J. Church , A. N. Parmar , M. Balucinska-Church , T. Mineo

We report results of a spectral and timing analysis of the poorly studied transient X-ray pulsar 2S 1553-542 using data collected with the NuSTAR and Chandra observatories and the Fermi/GBM instrument during an outburst in 2015. Properties…

Accreting X-ray pulsars (XRPs) undergo luminous X-ray outbursts during which the luminosity-dependent spectral and timing features of the neutron star's emission can be analyzed in detail, thus shedding light on the accretion regime at…

We report the identification of a bright hard X-ray source dominating the M31 bulge above 25 keV from a simultaneous NuSTAR-Swift observation. We find that this source is the counterpart to Swift J0042.6+4112, which was previously detected…

The main goal of this work is to perform a detailed study of the optical variability of the Be/X-ray binary SAX J2239.3+6116. We obtained multi-colour BVRI photometry and polarimetry and 4000-7000 A spectroscopy. The optical counterpart to…

太阳与恒星天体物理 · 物理学 2017-01-25 P. Reig , P. Blay , D. Blinov

We report a discovery of a new long-period X-ray pulsar SRGA J204318.2+443815/SRGe J204319.0+443820 in the Be binary system. The source was found in the second all-sky survey by the Mikhail Pavlinsky telescope on board the SRG mission. The…

Optical and near-infrared observations are compiled for the three gamma-ray binaries hosting Be stars: PSR B1259-63, LSI+61 303, and HESS J0632+057. The emissions from the Be disk are considered to vary according to the changes in its…

太阳与恒星天体物理 · 物理学 2021-09-03 Yuki Moritani , Akiko Kawachi

This work is devoted to the study of the broadband 0.8-79 keV spectral and timing properties of the poorly studied X-ray pulsar XTE J1859+083 during its 2015 outburst based on the data from the NuSTAR and Swift observatories. We show that…

(abridged) PSR J1048-5832 is a young Vela-like pulsar that was recently detected in gamma-rays with Fermi, and also in X-rays with Chandra and XMM-Newton. It powers a compact PWN visible in X-rays. We present deep optical observations with…

太阳与恒星天体物理 · 物理学 2013-04-17 Andrey Danilenko , Aida Kirichenko , Jesper Sollerman , Yury Shibanov , Dima Zyuzin

The EXTraS project to explore the X-ray Transient and variable Sky searches for coherent signals in the X-ray archival data of XMM-Newton. XMM-Newton performed more than 400 pointed observations in the region of the Large Magellanic Cloud…

We present an extended study of the Be/X-ray pulsar 2S 1553-542 during its Type II outbursts. We have incorporated \emph{NICER, Swift-XRT, RXTE-PCA, \emph{NuSTAR} and FERMI} observations to carry out the detailed phase and time resolved…

高能天体物理现象 · 物理学 2023-05-10 Binay Rai , Biswajit Paul , Mohammed Tobrej , Manoj Ghising , Ruchi Tamang , Bikash Chandra Paul

The emission-line Be star HD 215227 lies within the positional error circle of the newly identified gamma-ray source AGL J2241+4454. We present new blue spectra of the star, and we point out the morphological and variability similarities to…

太阳与恒星天体物理 · 物理学 2015-05-20 S. J. Williams , D. R. Gies , R. A. Matson , Y. Touhami , E. D. Grundstrom , W. Huang , M. V. McSwain
‹ 上一页 1 2 3 10 下一页 ›