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Related papers: Multiband Optical Light Curves of Black-Widow Puls…

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We present simultaneous, multi-colour optical light curves of the companion star to the black-widow pulsar PSR J2051-0827, obtained approximately 10 years apart using ULTRACAM and HiPERCAM, respectively. The ULTRACAM light curves confirm…

Black widows are extreme millisecond pulsar binaries where the pulsar wind ablates their low-mass companion stars. Their optical light curves vary periodically due to the high irradiation and tidal distortion of the companion, which allows…

High Energy Astrophysical Phenomena · Physics 2023-03-22 D. Mata Sánchez , M. R. Kennedy , C. J. Clark , R. P. Breton , V. S. Dhillon , G. Voisin , F. Camilo , S. Littlefair , T. R. Marsh , J. Stringer

We present an analysis of archival Gemini g', r', K and Keck H, K_s imaging of this nearby short period binary (P_B=95.8min) 2.87ms pulsar. The heated companion is clearly detected. Direct pulsar heating provides an acceptable model at the…

High Energy Astrophysical Phenomena · Physics 2018-08-08 Paul Draghis , Roger W. Romani

We present a model for atmospheric wind circulation in binary millisecond pulsar (MSP) companions, showing how the optical light curve (LC) and radial velocities (RV) are sensitive to the wind flow, causing LC orbital phase shifts and…

High Energy Astrophysical Phenomena · Physics 2020-04-08 D. Kandel , Roger W. Romani

We report the optical identification of the companion to the {\it Fermi} black widow millisecond pulsar PSR J1544+4937. We find a highly variable source on Keck LRIS images at the nominal pulsar position, with 2 magnitude variations over…

The low mass companions of evaporating binary pulsars (black widows and their ilk) are strongly heated on the side facing the pulsar. However in high-quality photometric and spectroscopic data the heating pattern does not match that…

High Energy Astrophysical Phenomena · Physics 2016-08-31 Roger W. Romani , Nicolas Sanchez

The optical study of the heated substellar companions of `Black Widow' (BW) millisecond pulsars (MSP) provides unique information on the MSP particle and radiation output and on the neutron star mass. Here we present analysis of optical…

High Energy Astrophysical Phenomena · Physics 2023-01-04 D. Kandel , Roger W. Romani

In the last few years, over 43 millisecond radio pulsars have been discovered by targeted searches of unidentified gamma-ray sources found by the Fermi Gamma-Ray Space Telescope. A large fraction of these millisecond pulsars are in compact…

High Energy Astrophysical Phenomena · Physics 2015-06-15 R. P. Breton , M. H. van Kerkwijk , M. S. E. Roberts , J. W. T. Hessels , F. Camilo , M. A. McLaughlin , S. M. Ransom , P. S. Ray , I. H. Stairs

We present ULTRACAM multiband optical photometry of two transitional millisecond pulsars, PSR J1023+0038 and PSR J1227$-$4853, taken while both were in their radio pulsar states. The light curves show significant asymmetry about the flux…

A large number of new "black widow" and "redback" energetic millisecond pulsars with irradiated stellar companions have been discovered through radio and optical searches of unidentified \textit{Fermi} sources. Synchrotron emission, from…

High Energy Astrophysical Phenomena · Physics 2016-02-23 Zorawar Wadiasingh , Alice K. Harding , Christo Venter , Markus Boettcher

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…

High Energy Astrophysical Phenomena · Physics 2015-06-18 Joshua Schroeder , Jules Halpern

We describe the first X-ray observations of five short orbital period ($P_B < 1$ day), $\gamma$-ray emitting, binary millisecond pulsars. Four of these, PSRs J0023+0923, J1124$-$3653, J1810+1744, and J2256$-$1024 are `black-widow' pulsars,…

High Energy Astrophysical Phenomena · Physics 2015-06-16 P. Gentile , M. Roberts , M. McLaughlin , F. Camilo , J. Hessels , M. Kerr , S. Ransom , P. Ray , I. Stairs

We present optical time-resolved multi-band photometry of the black widow binary millisecond pulsar J2052+1219 using direct-imaging observations with the 2.1m telescope of Observatorio Astronomico Nacional San Pedro Martir, Mexico…

Solar and Stellar Astrophysics · Physics 2019-10-02 S. Zharikov , A. Kirichenko , D. Zyuzin , Yu. Shibanov , J. S. Deneva

We have measured dramatic flux and spectral variations through the 0.193d orbit of the optical counterpart of the unidentified gamma-ray source 0FGL J2339.8-0530. This compact object companion is strongly heated, with T_eff varying from…

High Energy Astrophysical Phenomena · Physics 2015-06-03 Roger W. Romani , Michael S. Shaw

Using the 1.3m and 2.4m telescopes of the MDM Observatory, we identified the close companions of two eclipsing millisecond radio pulsars discovered by the Green Bank Telescope in searches of Fermi Gamma-ray Space Telescope sources, and…

High Energy Astrophysical Phenomena · Physics 2015-06-22 Miao Li , Jules P. Halpern , John R. Thorstensen

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…

High Energy Astrophysical Phenomena · Physics 2025-02-20 Marco Turchetta , Bidisha Sen , Jordan A. Simpson , Manuel Linares , Rene P. Breton , Jorge Casares , Mark R. Kennedy , Tariq Shahbaz

The companions of evaporating binary pulsars (black widows and related systems) show optical emission suggesting strong heating. In a number of cases large observed temperatures and asymmetries are inconsistent with direct radiative heating…

High Energy Astrophysical Phenomena · Physics 2017-08-23 Nicholas Sanchez , Roger W. Romani

Several redback and black widow millisecond pulsar binaries have episodes of flaring in X-rays and optical. We initially detected such behavior from the Fermi selected redback candidate 1FGL J0523.5$-$2529 during optical time-series…

High Energy Astrophysical Phenomena · Physics 2022-08-31 Jules P. Halpern , Karen I. Perez , Slavko Bogdanov

Hot subdwarfs in close binaries with either M dwarf, brown dwarf or white dwarf companions show unique light variations. In hot subdwarf binaries with M dwarf or brown dwarf companions we can observe the so-called reflection effect and in…

Solar and Stellar Astrophysics · Physics 2023-05-10 V. Schaffenroth , B. N. Barlow , I. Pelisoli , S. Geier , T. Kupfer
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