An atlas of burst oscillations and spectral properties in 4U 1728-34

被引:40
|
作者
van Straaten, S
van der Klis, M
Kuulkers, E
Méndez, M
机构
[1] Univ Amsterdam, Astron Inst Anton Pannekoek, NL-1098 SJ Amsterdam, Netherlands
[2] Ctr High Energy Astrophys, NL-1098 SJ Amsterdam, Netherlands
[3] Space Res Org Netherlands, NL-3584 CA Utrecht, Netherlands
[4] Univ Utrecht, Inst Astron, NL-3507 TA Utrecht, Netherlands
[5] Natl Univ La Plata, Fac Ciencias Astron & Geofis, RA-1900 La Plata, Argentina
来源
ASTROPHYSICAL JOURNAL | 2001年 / 551卷 / 02期
关键词
accretion; accretion disks; binaries : close; stars : individual (4U 1728-34); stars : neutron; X-rays : bursts; X-rays : stars;
D O I
10.1086/320234
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We study correlations between the burst properties and the position in the color-color diagram of the low mass X-ray binary 4U 1728-34 using 21 bursts found in two data sets obtained with the Rossi X-Ray Timing Explorer. Using spectral fits we analyze the spectral evolution during the bursts and determine the burst peak flux, temperature, rise time, and fluence. Using dynamical power spectra, we study the properties of the similar to 363 Hz burst oscillations. We find correlations between fluence, peak flux, the occurrence of radius expansion, and the presence of burst oscillations and the position of the source in the color-color diagram. The radius expansion bursts with and without burst oscillations differ both with respect to where they occur in the color-color diagram and in how the radius expansion takes place. We compare our results with those of a similar study by Muno and coworkers for KS 1731-26. Both KS 1731-260 and 4U 1728-34 show more or less the same behavior with respect to the dependence of the presence/absence of the burst oscillations on the position of the source in the color-color diagram, but the dependence of most of the spectral burst parameters on the position in the color-color diagram is clearly different. We find that the systematic absence in 4U 1728-34 of burst oscillations in the "island" state of the color-color diagram is not explained by the bursts involving mixed H-He burning, as Cumming & Bildsten found may be the case in KS 1731-260.
引用
收藏
页码:907 / 920
页数:14
相关论文
共 50 条
  • [1] Spectral analysis of the burst source 4U 1728-34
    Majczyna, A.
    Madej, J.
    Nalezyty, M.
    PHOTONICS APPLICATIONS IN ASTRONOMY, COMMUNICATIONS, INDUSTRY, AND HIGH-ENERGY PHYSICS EXPERIMENTS 2012, 2012, 8454
  • [2] NICER Observation of Unusual Burst Oscillations in 4U 1728-34
    Mahmoodifar, Simin
    Strohmayer, Tod E.
    Bult, Peter
    Altamirano, Diego
    Arzoumanian, Zaven
    Chakrabarty, Deepto
    Gendreau, Keith C.
    Guillot, Sebastien
    Homan, Jeroen
    Jaisawal, Gaurava K.
    Keek, Laurens
    Wolff, Michael T.
    ASTROPHYSICAL JOURNAL, 2019, 878 (02):
  • [3] The link between coherent burst oscillations, burst spectral evolution and accretion state in 4U 1728-34
    Zhang, Guobao
    Mendez, Mariano
    Zamfir, Michael
    Cumming, Andrew
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2016, 455 (02) : 2004 - 2017
  • [4] The effect of the mass accretion rate on the burst oscillations in 4U 1728-34
    Franco, LM
    ASTROPHYSICAL JOURNAL, 2001, 554 (01): : 340 - 351
  • [5] X-ray burst-induced spectral variability in 4U 1728-34
    Kajava, J. J. E.
    Sanchez-Fernandez, C.
    Kuulkers, E.
    Poutanen, J.
    ASTRONOMY & ASTROPHYSICS, 2017, 599
  • [6] On the nature of the compact star in 4U 1728-34
    Li, XD
    Ray, S
    Dey, J
    Dey, M
    Bombaci, I
    ASTROPHYSICAL JOURNAL, 1999, 527 (01): : L51 - L54
  • [7] Precise measurements of the kilohertz quasi-periodic oscillations in 4U 1728-34
    Méndez, M
    Van der Klis, M
    ASTROPHYSICAL JOURNAL, 1999, 517 (01): : L51 - L54
  • [8] RADIUS-EXPANSION BURST SPECTRA FROM 4U 1728-34: AN ULTRACOMPACT BINARY?
    Galloway, Duncan K.
    Yao, Yangsen
    Marshall, Herman
    Misanovic, Zdenka
    Weinberg, Nevin
    ASTROPHYSICAL JOURNAL, 2010, 724 (01): : 417 - 424
  • [9] The spectral states of the NS LMXB 4U 1728-34: pictures from a wider scenario
    Farinelli, R.
    Falanga, M.
    MULTICOLORED LANDSCAPE OF COMPACT OBJECTS AND THEIR EXPLOSIVE ORIGINS, 2007, 924 : 519 - +
  • [10] AstroSat/LAXPC Detection of Millisecond Phenomena in 4U 1728-34
    Chauhan, Jai Verdhan
    Yadav, J. S.
    Misra, Ranjeev
    Agrawal, P. C.
    Antia, H. M.
    Pahari, Mayukh
    Sridhar, Navin
    Dedhia, Dhiraj
    Katoch, Tilak
    Madhwani, P.
    Manchanda, R. K.
    Paul, B.
    Shah, Parag
    ASTROPHYSICAL JOURNAL, 2017, 841 (01):