Zobrazeno 1 - 9
of 9
pro vyhledávání: '"Andrew G. Cantrell"'
Autor:
Sera Markoff, James Miller-Jones, Rob Fender, Elena Gallo, Jeroen Homan, Piergiorgio Casella, P. Gandhi, Dipankar Maitra, David M. Russell, T. Shahbaz, Ritaban Chatterjee, Kieran O'Brien, Andrew G. Cantrell
Publikováno v:
ResearcherID
Monthly Notices of the Royal Astronomical Society, 429(1), 815-832. Oxford University Press
Monthly Notices of the Royal Astronomical Society, 429(1), 815-832. Oxford University Press
In X-ray binaries, compact jets are known to commonly radiate at radio to infrared frequencies, whereas at optical to gamma-ray energies, the contribution of the jet is debated. The total luminosity, and hence power of the jet is critically dependent
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ebe97bd256b2f8b19363b6cbaee19348
https://dare.uva.nl/personal/pure/en/publications/jet-spectral-breaks-in-black-hole-xray-binaries(5a5283c9-6dab-4bde-9366-6bf1058235c2).html
https://dare.uva.nl/personal/pure/en/publications/jet-spectral-breaks-in-black-hole-xray-binaries(5a5283c9-6dab-4bde-9366-6bf1058235c2).html
Autor:
Andrew G. Cantrell, Charles D. Bailyn, Heino Falcke, Sera Markoff, Dipankar Maitra, Jon D. Miller
Publikováno v:
Proceedings of the International Astronomical Union, 6(S275), 82-86. Cambridge University Press
We present results of recent observations and theoretical modeling of data from black holes accreting at very low luminosities (L/L_Edd ~ 10^{-8}). We discuss our newly developed time-dependent model for episodic ejection of relativistic plasma withi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::54ac4d5f79d4243a99e98e277a663f7d
https://doi.org/10.1017/S174392131001567X
https://doi.org/10.1017/S174392131001567X
Autor:
Andrew G. Cantrell, Ronald A. Remillard, Cynthia S. Froning, Dawn M. Gelino, Joseph Neilsen, Charles D. Bailyn, Jeffrey E. McClintock, Lijun Gou, Jerome A. Orosz
Publikováno v:
The Astrophysical Journal. 710:1127-1141
We analyze photometry of the Soft X-ray Transient A0620-00 spanning nearly 30 years, including previously published and previously unpublished data. Previous attempts to determine the inclination of A0620 using subsets of these data have yielded a wi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::766b1d154f0057d67e77b0a29325b09d
https://doi.org/10.1088/0004-637x/710/2/1127
https://doi.org/10.1088/0004-637x/710/2/1127
Publikováno v:
The Astrophysical Journal. 673:L159-L162
We present optical and infrared photometry of the soft X-ray transient A0620–00, obtained by the SMARTS and YALO consortia, spanning the period 1999-2007. Although A0620–00 was X-ray quiescent throughout this period, our data show three distinct
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::dfe65f52e13ea1381d4bf9bd324772ed
https://doi.org/10.1086/528793
https://doi.org/10.1086/528793
Autor:
Charles D. Bailyn, Ross Kennedy-Shaffer, Rachel K. D. MacDonald, Jerome A. Orosz, Jean H. Swank, Michelle Buxton, Craig B. Markwardt, Ritaban Chatterjee, Andrew G. Cantrell
We examine ~10 years of photometric data and find that the black hole X-ray binary V4641 Sgr has two optical states, passive and active, during X-ray quiescence. The passive state is dominated by ellipsoidal variations and is stable in the shape and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9489f6bb92fa1444fb471dd194ab7dde
http://arxiv.org/abs/1401.4190
http://arxiv.org/abs/1401.4190
Autor:
Cynthia S. Froning, Andrew G. Cantrell, Thomas J. Maccarone, Kevin France, Juthika Khargharia, Lisa M. Winter, Edward L. Robinson, Robert I. Hynes, Jess W. Broderick, Sera Markoff, Manuel A. P. Torres, Michael Garcia, Charles D. Bailyn, J. Xavier Prochaska, Jessica Werk, Chris Thom, Stéphane Béland, Charles W. Danforth, Brian Keeney, James C. Green
Publikováno v:
Astrophysical Journal, 743. IOP Publishing Ltd.
[Abridged.] We present multiwavelength observations of the black hole binary system, A0620-00. Using the Cosmic Origins Spectrograph on the Hubble Space Telescope, we have obtained the first FUV spectrum of A0620-00. The observed spectrum is flat in
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4af77f273264933e928d19bca07a8670
Autor:
Vicky Kalogera, Andrew G. Cantrell, Will M. Farr, Charles D. Bailyn, Niharika Sravan, Ilya Mandel, Laura Kreidberg
We perform a Bayesian analysis of the mass distribution of stellar-mass black holes using the observed masses of 15 low-mass X-ray binary systems undergoing Roche lobe overflow and five high-mass, wind-fed X-ray binary systems. Using Markov Chain Mon
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bb31774619588f515c27ca07f5dc3eab
http://arxiv.org/abs/1011.1459
http://arxiv.org/abs/1011.1459
Autor:
Andrew G. Cantrell, Charles D. Bailyn, James F. Steiner, Jerome A. Orosz, Ramesh Narayan, Jeffrey E. McClintock, Lijun Gou
During its yearlong outburst in 1975--76, the transient source A0620--00 reached an intensity of 50 Crab, an all-time record for any X-ray binary. The source has been quiescent since. We recently determined accurate values for the black hole mass, or
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b84e353e38029c7cc035142cecc31e85
http://arxiv.org/abs/1002.2211
http://arxiv.org/abs/1002.2211
Autor:
Andrew G. Cantrell, Charles D. Bailyn, Jeffrey E. McClintock, Jerome A. Orosz, Reba M. Bandyopadhyay, Stefanie Wachter, Dawn Gelino, Christopher R. Gelino
Publikováno v:
AIP Conference Proceedings.
We present optical and infrared photometry of the soft X‐ray transient A0620–00, obtained by the SMARTS and YALO consortia, spanning from 1999–2007. Although A0620–00 was X‐ray quiescent throughout this period, our data show three distinct
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::fdf81ecda699e904484ec0ead0405efd
https://doi.org/10.1063/1.2945092
https://doi.org/10.1063/1.2945092