UKIRT IR spectra of the microquasar GRS 1915+105

被引：0
|
作者：
Harlaftis, E
Dhillon, VS
Castro-Tirado, AJ
机构：
[1] Natl Observ Athens, Inst Astron & Astrophys, Athens 11810, Greece
[2] Univ Sheffield, Dept Phys & Astron, Sheffield S3 7RH, S Yorkshire, England
[3] CSIC, Inst Astrofis Andalucia, E-18080 Granada, Spain
[4] INTA, LAEFF, E-28080 Madrid, Spain
来源：
ASTROPHYSICS AND SPACE SCIENCE | 2001年 / 276卷 / Suppl 1期
关键词：
D O I：
10.1023/A:1011651213950
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The UKIRT JHK-band spectrum of GRS 1915+105 shows strong He I (2.059 mum) and Br gamma (2.166 mum) emission lines. Eikenberry et al. (1998) found flux variations of a factor of 5 in these lines on a 5 min timescale. Based on the detection or not of the He II emission line, it was suggested that the companion could be a LMXB or a HMXB, respectively, Since the spectral type of the companion star of GRS 1915+105 is still an open question,ve attempt to clarify the issue by revisiting the object and comparing the JHK spectrum with that of the Be star DM +49 3718 and the prototype X-ray binary Sco X-1.
引用
收藏
页码：35 / 38
页数：4
相关论文
共 50 条
  • [31] Observations of rapid disk-jet interaction in the microquasar GRS 1915+105
    Rothstein, DM
    Eikenberry, SS
    Matthews, K
    ASTROPHYSICAL JOURNAL, 2005, 626 (02): : 991 - 1005
  • [32] HST NICMOS observations of fast infrared flickering in the microquasar GRS 1915+105
    Eikenberry, Stephen S.
    Patel, Shannon G.
    Rothstein, David M.
    Remillard, Ronald
    Pooley, Guy G.
    Morgan, Edward H.
    ASTROPHYSICAL JOURNAL, 2008, 678 (01): : 369 - 375
  • [33] Spectral modeling of the three spectral states of the Galactic microquasar GRS 1915+105
    Zycki, P.T. (ptz@camk.edu.pl), 1600, EDP Sciences (400):
  • [34] Coupling between the accreting corona and the relativistic jet in the microquasar GRS 1915+105
    Mendez, Mariano
    Karpouzas, Konstantinos
    Garcia, Federico
    Zhang, Liang
    Zhang, Yuexin
    Belloni, Tomaso M.
    Altamirano, Diego
    NATURE ASTRONOMY, 2022, 6 (05) : 577 - 583
  • [35] Coupling between the accreting corona and the relativistic jet in the microquasar GRS 1915+105
    Mariano Méndez
    Konstantinos Karpouzas
    Federico García
    Liang Zhang
    Yuexin Zhang
    Tomaso M. Belloni
    Diego Altamirano
    Nature Astronomy, 2022, 6 : 577 - 583
  • [36] Accretion disk winds as the jet suppression mechanism in the microquasar GRS 1915+105
    Neilsen, Joseph
    Lee, Julia C.
    NATURE, 2009, 458 (7237) : 481 - 484
  • [37] Accretion disk winds as the jet suppression mechanism in the microquasar GRS 1915+105
    Joseph Neilsen
    Julia C. Lee
    Nature, 2009, 458 : 481 - 484
  • [38] Spectral modeling of the three spectral states of the Galactic microquasar GRS 1915+105
    Sobolewska, MA
    Zycki, PT
    ASTRONOMY & ASTROPHYSICS, 2003, 400 (02) : 553 - 558
  • [39] BeppoSAX observation of the microquasar GRS 1915+105: spectral and timing behavior in the ρ class
    Mineo, T.
    Massaro, E.
    Cusumano, G.
    X-RAY ASTRONOMY-2009: PRESENT STATUS, MULTI-WAVELENGTH APPROACH AND FUTURE PERSPECTIVES, PROCEEDINGS, 2010, 1248 : 183 - +
  • [40] Phase lags of quasi-periodic oscillations in microquasar GRS 1915+105
    Cui, W
    ASTROPHYSICAL JOURNAL, 1999, 524 (01): : L59 - L62
12345