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相关论文: 4FGL J1120.0-2204: A Unique Gamma-ray Bright Neutr…

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On 2009 June 5, the Gamma-ray Burst Monitor (GBM) onboard the Fermi Gamma-ray Space Telescope triggered on two short, and relatively dim bursts with spectral properties similar to Soft Gamma Repeater (SGR) bursts. Independent localizations…

Low-mass white dwarfs can either be produced in low-mass X-ray binaries by stable mass transfer to a neutron star, or in a common-envelope phase with a heavier white dwarf companion. We have searched 8 low-mass white dwarf candidates…

天体物理学 · 物理学 2008-11-26 Joeri van Leeuwen , Robert D. Ferdman , Sol Meyer , Ingrid Stairs

We describe the first X-ray observations of binary millisecond pulsars PSRs J0023+0923, J1810+1744, J2215+5135, and J2256-1024. All four are Fermi gamma-ray sources and three are 'black-widow' pulsars, with companions of mass < 0.1 solar…

太阳与恒星天体物理 · 物理学 2015-06-11 Peter Gentile , Maura McLaughlin , Mallory Roberts , Fernando Camilo , Jason Hessels , Matthew Kerr , Scott Ransom , Paul Ray , Ingrid Stairs

Aims. We aim to contribute to the identification of unassociated gamma-ray sources in the galactic plane in order to enlarge the currently known population of gamma-ray binaries and related systems, such as radio emitting X-ray binaries and…

Symbiotic X-ray binaries form a subclass of low-mass X-ray binary systems consisting of a neutron star accreting material from a red giant donor star via stellar wind or Roche lobe overflow. Only a few confirmed members are currently known;…

高能天体物理现象 · 物理学 2015-06-18 A. A. Nucita , S. Stefanelli , F. De Paolis , N. Masetti , G. Ingrosso , M. Del Santo , L. Manni

I obtained time-series photometry of the compact binary candidate for the Fermi source 4FGL J0935.3+0901. Superposed on the 2.44 hr orbital modulation are day-to-day variations and frequent flaring as seen in several redback and black widow…

高能天体物理现象 · 物理学 2022-07-19 J. P. Halpern

We present the detection of the binary system 2MASS J02132062+3648506 AB using the Karl G. Jansky Very Large Array (VLA) archive data observed at 4-8 GHz. The system is a triple consisting of a tight binary ($\sim0.2"$) of two M dwarfs of…

We report on the results of the multiwavelength campaign carried out after the discovery of the INTEGRAL transient IGR J17329-2731. The optical data collected with the SOAR telescope allowed us to identify the donor star in this system as a…

高能天体物理现象 · 物理学 2018-03-06 E. Bozzo , A. Bahramian , C. Ferrigno , A. Sanna , J. Strader , F. Lewis , D. M. Russell , T. di Salvo , L. Burderi , A. Riggio , A. Papitto , P. Gandhi , P. Romano

We present the discovery of a companion to the Y-dwarf, CWISEP J193518.59-154620.3, the second Y-Y dwarf binary detected to date. Y-dwarfs are the coldest known free-floating objects ($<$ 500 K) and on average represent the lowest mass…

We report the detection of a possible gamma-ray counterpart of the accreting millisecond pulsar SAX J1808.4-3658. The analysis of ~6 years of data from the Large Area Telescope on board the Fermi Gamma-ray Space Telescope (Fermi-LAT) within…

高能天体物理现象 · 物理学 2016-01-27 E. de Ona Wilhelmi , A. Papitto , J. Li , N. Rea , D. F. Torres , L. Burderi , T. Di Salvo , R. Iaria , A. Riggio , A. Sanna

We searched for radio pulsars in 25 of the non-variable, unassociated sources in the Fermi LAT Bright Source List with the Green Bank Telescope at 820 MHz. We report the discovery of three radio and gamma-ray millisecond pulsars (MSPs) from…

We present a multi-band search for X-ray, optical and $\gamma$-ray emission of the radio binary millisecond pulsar J1836-2354A, hosted in the globular cluster M22. X-ray emission is significantly detected in two Chandra observations,…

高能天体物理现象 · 物理学 2019-04-24 R. Amato , A. D'Aì , M. Del Santo , D. de Martino , A. Marino , T. Di Salvo , R. Iaria , T. Mineo

In a search with the Parkes radio telescope of 56 unidentified Fermi-LAT gamma-ray sources, we have detected 11 millisecond pulsars (MSPs), 10 of them discoveries, of which five were reported in Kerr et al. (2012). We did not detect radio…

We present optical high-speed photometry of three millisecond pulsars with low-mass ($< 0.3 M_{\odot}$) white dwarf companions, bringing the total number of such systems with follow-up time-series photometry to five. We confirm the…

The recycled pulsar PSR J2222-0137 is one of the closest known neutron stars, with a parallax distance of $267_{-0.9}^{+1.2}\,$pc and an edge-on orbit. We measure the Shapiro delay in the system through pulsar timing with the Green Bank…

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 present observations of a new very low mass field binary, discovered during an infrared imaging survey of 250 DENIS L and very late-M dwarfs. DENIS-J055146.0-443412.2 is an M8.5+L0 pair, with a physical separation of over 200 AU. This…

天体物理学 · 物理学 2009-11-11 M. Billeres , X. Delfosse , J. -L. Beuzit , T. Forveille , L. Marchal , E. L. Martin

PSR J1738+0333 is one of the four millisecond pulsars known to be orbited by a white dwarf companion bright enough for optical spectroscopy. Of these, it has the shortest orbital period, making it especially interesting for a range of…

高能天体物理现象 · 物理学 2012-07-11 J. Antoniadis , M. H. van Kerkwijk , D. Koester , P. C. C. Freire , N. Wex , T. M. Tauris , M. Kramer , C. G. Bassa

We report on observations of the unusual neutron-star binary system FIRST J102347.6+003841 carried out using the XMM-Newton satellite. This system consists of a radio millisecond pulsar in an 0.198-day orbit with a ~0.2 solar-mass…

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…