English
Related papers

Related papers: Chandra Observations of Black-Widow Pulsars

200 papers

PSR J0108-1431 is a nearby, 170 Myr old, very faint radio pulsar near the "pulsar death line" in the P-Pdot diagram. We observed the pulsar field with the Chandra X-ray Observatory and detected a point source (53 counts in a 30 ks exposure,…

Astrophysics · Physics 2009-06-23 G. G. Pavlov , O. Kargaltsev , J. A. Wong , G. P. Garmire

We report on 22 yrs of radio timing observations of the millisecond pulsar J1024$-$0719 by the telescopes participating in the European Pulsar Timing Array (EPTA). These observations reveal a significant second derivative of the pulsar spin…

We analysed Chandra observations of the bright Fermi pulsar J0633+0632 and found evidence of an absorption feature in its spectrum at $804^{+42}_{-26}$ eV (the errors here and below are at 90% confidence) with equivalent width of…

High Energy Astrophysical Phenomena · Physics 2015-12-14 Andrey Danilenko , Peter Shternin , Anna Karpova , Dima Zyuzin , Yuriy Shibanov

We present an analysis of 745.6 ks of archival Chandra X-ray Observatory Advanced CCD Imaging Spectrometer data accumulated between 2000 and 2016 of the millisecond pulsar (MSP) population in the rich Galactic globular cluster Terzan 5.…

High Energy Astrophysical Phenomena · Physics 2021-05-19 Slavko Bogdanov , Arash Bahramian , Craig O. Heinke , Scott M. Ransom

We report on the follow-up $XMM-Newton$ observation of the persistent X-ray pulsar CXOU J225355.1+624336, discovered with the CATS@BAR project on archival $Chandra$ data. The source was detected at $f_{\rm X}$(0.5-10 keV) = 3.4$\times…

High Energy Astrophysical Phenomena · Physics 2021-05-26 N. La Palombara , L. Sidoli , P. Esposito , G. L. Israel , G. A. Rodríguez Castillo

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…

We report the discovery of two millisecond pulsars in a search for radio pulsations at the positions of \emph{Fermi Large Area Telescope} sources with no previously known counterparts, using the Nan\c{c}ay radio telescope. The two…

We report the detection of the millisecond pulsar B1257+12 with the Chandra X-ray Observatory. In a 20 ks exposure we detected 25 photons from the pulsar, with energies between 0.4 and 2.0 keV, corresponding to the flux F_X=(4.4+/-…

Astrophysics · Physics 2009-06-23 G. G. Pavlov , O. Kargaltsev , G. P. Garmire , A. Wolszczan

We observed the field of the Fermi source 3FGL J0838.8-2829 in optical and X-rays, initially motivated by the cataclysmic variable (CV) 1RXS J083842.1-282723 that lies within its error circle. Several X-ray sources first classified as CVs…

High Energy Astrophysical Phenomena · Physics 2017-04-05 Jules P. Halpern , Slavko Bogdanov , John R. Thorstensen

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…

PSR B0628-28 is an X-ray emitting radio pulsar which was observed with Advanced CCD Imaging Spectrometer (ACIS) on board Chandra on 2001 November 04 and on 2002 March 25 for 2000 s and 17000 s, respectively. The source countrate was…

Astrophysics · Physics 2007-05-23 Hakki Ogelman , Emre Tepedelenlioglu

We report multi-wavelength observations of the unidentified Fermi object 2FGL J1653.6-0159. With the help of high-resolution X-ray observation, we have identified an X-ray and optical counterpart of 2FGL J1653.6-0159. The source exhibits a…

High Energy Astrophysical Phenomena · Physics 2015-06-22 A. K. H. Kong , R. Jin , T. -C. Yen , C. P. Hu , C. Y. Hui , P. H. T. Tam , J. Takata , L. C. C. Lin , K. S. Cheng , S. M. Park , C. L. Kim

We study the timing stability of three black widow pulsars, both in terms of their long-term spin evolution and their shorter-term orbital stability. The erratic timing behaviour and radio eclipses of the first two black widow pulsar…

We report on spectral and timing observations of the nearest millisecond pulsar J0437-4715 with Chandra. The pulsar spectrum, detected up to 7 keV, cannot be described by a simple one-component model. We suggest that it consists of two…

Astrophysics · Physics 2009-11-07 V. E. Zavlin , G. G. Pavlov , D. Sanwal , R. N. Manchester , J. Truemper , J. P. Halpern , W. Becker

The middle-aged PSR J0357+3205 is a nearby, radio-quiet, bright gamma-ray pulsar discovered by the Fermi mission. Our previous Chandra observation revealed a huge, very peculiar structure of diffuse X-ray emission, originating at the pulsar…

High Energy Astrophysical Phenomena · Physics 2015-06-12 A. De Luca , R. P. Mignani , M. Marelli , D. Salvetti , N. Sartore , A. Belfiore , P. Saz Parkinson , P. A. Caraveo , G. F. Bignami

Millisecond pulsars (MSPs) are faint X-ray sources commonly observed in Galactic globular clusters (GCs). In this work, we investigate 18 MSPs newly found in the GC Omega Centauri ($\omega$ Cen) and search for their X-ray counterparts using…

High Energy Astrophysical Phenomena · Physics 2023-09-26 Jiaqi Zhao , Craig O. Heinke

'Spider' binary systems - black widow and redback compact binaries differentiated by their companion's mass and nature - are an important type of pulsar system exhibiting a rich empirical phenomenology, including radio eclipses, optical…

High Energy Astrophysical Phenomena · Physics 2026-02-12 Christo Venter , Andreas Kopp , Zorawar Wadiasingh , Alice K Harding , M Baring

We report here the results obtained from a systematic optical photometric survey aimed at finding new compact binary millisecond pulsars (also known as "spiders"): the COmpact BInary PULsar SEarch (COBIPULSE). We acquired multi-band optical…

We report on a timing and spectral analysis of the young, high magnetic field rotation-powered pulsar (RPP) B1509-58 using Chandra continuous-clocking mode observation. The pulsar's X-ray light curve can be fit by the two Gaussian…

High Energy Astrophysical Phenomena · Physics 2017-04-12 Chin-Ping Hu , C. -Y. Ng , J. Takata , R. M. Shannon , S. Johnston

PSR J1641+8049 is a 2 ms black widow pulsar with the 2.2 h orbital period detected in the radio and $\gamma$-rays. We performed new phase-resolved multi-band photometry of PSR J1641+8049 using the OSIRIS instrument at the Gran Telescopio…

‹ Prev 1 8 9 10 Next ›