SWIFT J1753.5-0127: orbital period, high-frequency timing analysis and multi-band observations

被引：0

作者：

Durant, Martin ^{[1
]}

Shahbaz, Tariq ^{[1
]}

Zurita, Cristina ^{[1
]}

Torres, Manuel A. P. ^{[1
]}

机构：

[1] Inst Astrofis Canarias, C Via Lactea S-N, E-38205 San Cristobal la Laguna, Tenerife, Spain

来源：

UNIVERSE AT SUB-SECOND TIMESCALES: HIGH TIME RESOLUTION ASTROPHYSICS | 2008年 / 984卷

关键词：

black hole candidate; high-frequency timing; multi-band photometry;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We have conducted an extensive observational campaign of SWIFT J1753.5-0127 over the last year, since its bright our-burst episode in 2005. Using long time baseline optical photometry, we have found a new period suggestive of orbital modulation with a period of 3.2 h, we have simultaneous multi-band photometry, and high-frequency multi-band photometry from ULTRACAM. In the latter data, we find evidence for a broad quasi-periodic oscillation in the g' and r' bands centred on a period of similar to 25 s and a narrower one of period similar to 12 s.

引用

页码：256 / +

页数：2

共 21 条

[1] MULTIWAVELENGTH OBSERVATIONS OF Swift J1753.5-0127
Froning, Cynthia S.
Maccarone, Thomas J.
France, Kevin
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Robinson, Edward L.
Hynes, Robert I.
Lewis, Fraser
ASTROPHYSICAL JOURNAL, 2014, 780 (01):
[2] Swift J1753.5-0127: The black hole candidate with the shortest orbital period
Zurita, C.
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Torres, M. A. P.
Shahbaz, T.
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Steeghs, D.
ASTROPHYSICAL JOURNAL, 2008, 681 (02): : 1458 - 1463
[3] Multiwavelength observations of the black hole candidate Swift J1753.5-0127
Soleri, P.
Altamirano, D.
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Maitra, D.
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POPULATION EXPLOSION: THE NATURE AND EVOLUTION OF X-RAY BINARIES IN DIVERSE ENVIRONMENTS, 2008, 1010 : 103 - +
[4] Multiwavelength spectral and high time resolution observations of SWIFT J1753.5-0127: new activity?
Durant, M.
Gandhi, P.
Shahbaz, T.
Peralta, H. H.
Dhillon, V. S.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2009, 392 (01) : 309 - 324
[5] Swift J1753.5-0127: understanding the accretion geometry through frequency-resolved spectroscopy
Blessy E. Baby
M. C. Ramadevi
Journal of Astrophysics and Astronomy, 2022, 43
[6] Swift J1753.5-0127: understanding the accretion geometry through frequency-resolved spectroscopy
Baby, Blessy E.
Ramadevi, M. C.
JOURNAL OF ASTROPHYSICS AND ASTRONOMY, 2022, 43 (01)
[7] Expanding hot flow in the black hole binary SWIFT J1753.5-0127: evidence from optical timing
Veledina, Alexandra
Gandhi, Poshak
Hynes, Robert
Kajava, Jari J. E.
Tsygankov, Sergey S.
Revnivtsev, Michail G.
Durant, Martin
Poutanen, Juri
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2017, 470 (01) : 48 - 59
[8] Accretion flow diagnostics with X-ray spectral timing: the hard state of SWIFT J1753.5-0127
Cassatella, P.
Uttley, P.
Maccarone, T. J.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2012, 427 (04) : 2985 - 2997
[9] SWIFT X-RAY TELESCOPE TIMING OBSERVATIONS OF THE BLACK HOLE BINARY SWIFT J1753.5-0127: DISK-DILUTED FLUCTUATIONS IN THE OUTBURST PEAK
Kalamkar, M.
van der Klis, M.
Uttley, P.
Altamirano, Diego
Wijnands, Rudy
ASTROPHYSICAL JOURNAL, 2013, 766 (02):
[10] Simultaneous multiwavelength observations of the low/hard state of the X-ray transient source SWIFT J1753.5-0127
Bel, M. Cadolle
Ribo, M.
Rodriguez, J.
Chaty, S.
Corbel, S.
Goldwurm, A.
Frontera, F.
Farinelli, R.
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Tarana, A.
Ubertini, P.
Laurent, P.
Goldoni, P.
Mirabel, I. F.
ASTROPHYSICAL JOURNAL, 2007, 659 (01): : 549 - 560

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