Zobrazeno 1 - 10
of 34
pro vyhledávání: '"Bram Boroson"'
Autor:
John M. Dickey, S. D. Vrtilek, Michael McCollough, Bram Boroson, John A. Tomsick, Charles Bailyn, Jay M. Blanchard, Charlotte Johnson
Publikováno v:
The Astrophysical Journal Supplement Series, Vol 268, Iss 1, p 35 (2023)
The rapid variability of X-ray binaries (XRBs) produces a wide range of X-ray states that are linked to activity across the electromagnetic spectrum. It is particularly challenging to study a sample of sources large enough to include all types in the
Externí odkaz:
https://doaj.org/article/85c0f66a144a470194505e49d61b87c7
Autor:
Ewan O'Sullivan, A. Mossman, Jennifer Lauer, Raffaele D'Abrusco, Ginevra Trinchieri, Giuseppina Fabbiano, Douglas Morgan, Douglas Burke, Nazma Islam, Bram Boroson, C. Anderson, S. D. Vrtilek, Michael L. McCollough, Alessandro Paggi, Dong-Woo Kim, Antonella Fruscione
X-ray binaries exhibit a wide range of properties but there are few accepted methods to determine the nature of the compact object. Color-Color-Intensity diagrams have been suggested as a means of distinguishing between systems containing black holes
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bf1cde07ff231881e8c1b6f528c3c277
Autor:
Saeqa Dil Vrtilek, Bram Boroson
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 428:3693-3714
Publikováno v:
The Astrophysical Journal. 720:1202-1214
We present results from spectral and temporal analyses of Suzaku and RXTE observations of the high mass X-ray binary LMC X-4. Using the full 13 years of available RXTE/ASM data, we apply the ANOVA and Lomb normalized Periodogram methods to obtain an
Autor:
Saeqa Dil Vrtilek, Bram Boroson
Publikováno v:
The Astrophysical Journal. 710:197-206
Orbital variability has been found in the X-ray hardness of the black hole candidate Cygnus X-1 during the soft/high X-ray state using light curves provided by the Rossi X-ray Timing Explorer's All Sky Monitor. We are able to set broad limits on how
Publikováno v:
The Astrophysical Journal. 678:1248-1262
High-resolution ultraviolet observations of Cygnus X-1 were obtained at two epochs roughly 1 year apart using the Space Telescope Imaging Spectrograph on the Hubble Space Telescope. Orbital phase ranges around orb = 0 and 0.5 were covered at each epo
Publikováno v:
The Astrophysical Journal. 626:307-316
We present a detailed spectral analysis of Chandra/ACIS-S CC mode observations of the massive X-ray binary system SMC X-1. The system was observed during both the high and low X-ray states of the roughly 60-day superorbital period. The continuum spec
Publikováno v:
Astronomische Nachrichten. 325:209-212
The Space Telescope Imaging Spectrograph (STIS) on HST provides the first ultraviolet data that are of sufficient spectral and temporal resolution to generate Doppler tomograms of X-ray binaries.We show both optical and ultraviolet maps constructed f
Publikováno v:
The Astrophysical Journal. 583:861-877
We analyze observations of the low-mass X-ray binary (LMXB) 2S 0921-63 obtained with the gratings and CCDs on Chandra and XMM. This object is a high-inclination system showing evidence for an accretion disk corona (ADC). Such a corona has the potenti
Publikováno v:
Publications of the Astronomical Society of the Pacific. 114:340-349
We present an archival study of ultraviolet spectra of the X-ray binary LMC X-4 obtained with the IUE satellite. We fit these spectra with models that incorporate the X-ray heating of the O star and accretion disk. A systematic analysis of the UV con