The outburst radial velocity curve of X-ray Nova Scorpii 1994 (= GRO J1655-40): a reduced mass for the black hole?

被引：34

作者：

Phillips, SN ^{[1
]}

Shahbaz, T ^{[1
]}

Podsiadlowski, P ^{[1
]}

机构：

[1] Univ Oxford, Dept Astrophys, Oxford OX1 3RH, England

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1999年 / 304卷 / 04期

关键词：

accretion; accretion discs; binaries : close; stars : individual : X-ray Nova Sco 1994 (GRO J1655-40); X-rays : stars;

D O I：

10.1046/j.1365-8711.1999.02357.x

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present a re-analysis of the outburst radial velocity data for X-ray Nova Scorpii 1994. Using a model based on X-ray heating of the secondary star, we suggest a more realistic treatment of the radial velocity data. Solutions are obtained in the (K-2,q) plane which, when combined with the published value for the binary mass ratio and inclination, constrain the mass of the black hole to within the region 4.1 < M-1 < 6.6 M-. (90 per cent confidence), which is significantly lower than the value obtained by Orosz & Bailyn, This reduced lower bound for the black hole mass, together with the high space velocity of the system, is consistent with the idea that it was formed by the post-supernova collapse of a neutron star.

引用

页码：839 / 844

页数：6

共 50 条

[31] Canonical black hole states in the superluminal source GRO J1655-40
Mendez, M
Belloni, T
van der Klis, M
ASTROPHYSICAL JOURNAL, 1998, 499 (02): : L187 - L190
[32] Supernova Archaeology with X-Ray Binary Winds: The Case of GRO J1655-40
Keshet, Noa
Behar, Ehud
Kallman, Timothy R.
ASTROPHYSICAL JOURNAL, 2024, 966 (02):
[33] CONTROVERSY OF THE GRO J1655-40 BLACK HOLE MASS AND SPIN ESTIMATES AND ITS POSSIBLE SOLUTIONS
Stuchlik, Z.
Kolos, M.
ASTROPHYSICAL JOURNAL, 2016, 825 (01):
[34] EPISODIC EJECTION OF RELATIVISTIC JETS BY THE X-RAY TRANSIENT GRO J1655-40
HJELLMING, RM
RUPEN, MP
NATURE, 1995, 375 (6531) : 464 - 468
[35] CORRELATIONS BETWEEN X-RAY OUTBURSTS AND RELATIVISTIC EJECTIONS IN THE X-RAY TRANSIENT GRO J1655-40
HARMON, BA
WILSON, CA
ZHANG, SN
PACIESAS, WS
FISHMAN, GJ
HJELLMING, RM
RUPEN, MP
SCOTT, DM
BRIGGS, MS
RUBIN, BC
NATURE, 1995, 374 (6524) : 703 - 706
[36] Swift Spectroscopy of the Accretion Disk Wind in the Black Hole GRO J1655-40
Balakrishnan, M.
Miller, J. M.
Trueba, N.
Reynolds, M.
Raymond, J.
Proga, D.
Fabian, A. C.
Kallman, T.
Kaastra, J.
ASTROPHYSICAL JOURNAL, 2020, 893 (02):
[37] A HYBRID MAGNETICALLY/THERMALLY DRIVEN WIND IN THE BLACK HOLE GRO J1655-40?
Neilsen, Joseph
Homan, Jeroen
ASTROPHYSICAL JOURNAL, 2012, 750 (01):
[38] Optical observations of GRO J1655-40 in quiescence .1. A precise mass for the black hole primary
Orosz, JA
Bailyn, CD
ASTROPHYSICAL JOURNAL, 1997, 477 (02): : 876 - 896
[39] Models of quasi-periodic oscillations related to mass and spin of the GRO J1655-40 black hole
Stuchlik, Zdenek
Kolos, Martin
ASTRONOMY & ASTROPHYSICS, 2016, 586
[40] Testing the nature of the black hole candidate in GRO J1655-40 with the relativistic precession model
Cosimo Bambi
The European Physical Journal C, 2015, 75

← 1 2 3 4 5 →