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Related papers: Optical Spectroscopy of GRO J1655-40

200 papers

We present twelve epochs of optical spectroscopy taken across the discovery outburst of the black hole candidate MAXI J1803-298 with the GTC and VLT telescopes. The source followed a standard outburst evolution with hard and soft states.…

We present ellipsoidal light-curve fits to the quiescent B, V, R and I light curves of GRO J1655-40 (Nova Scorpii 1994). The fits are based on a simple model consisting of a Roche-lobe filling secondary and an accretion disc around the…

Astrophysics · Physics 2009-11-07 Martin E. Beer , Philipp Podsiadlowski

We report results from the X-ray and optical monitoring of the black hole candidate MAXI J1820+070 (=ASSASN-18ey) over the entire period of its outburst from March to October 2018.In this outburst, the source exhibited two sets of `fast…

High Energy Astrophysical Phenomena · Physics 2019-04-17 Megumi Shidatsu , Satoshi Nakahira , Katsuhiro L. Murata , Ryo Adachi , Nobuyuki Kawai , Yoshihiro Ueda , Hitoshi Negoro

We present the discovery of an optical accretion disk wind in the X-ray transient Swift J1858.6-0814. Our 90-spectrum data set, taken with the 10.4m GTC telescope over 8 different epochs and across five months, reveals the presence of…

A comparison is made between the properties of CAL 83, CAL 87, RX J0513.9-6951, 1E 0035.4-7230 (SMC 13), RX J0019.8+2156, and RX J0925.7-4758, all supersoft X-ray binaries. Spectra with the same resolution and wavelength coverage of these…

Astrophysics · Physics 2016-08-30 A. P. Cowley , P. C. Schmidtke , D. Crampton , J. B. Hutchings

The present paper describes the analysis of multiple RXTE/PCA data of the black hole binary with superluminal jet, XTE J1550-564, acquired during its 1999--2000 outburst. The X-ray spectra show features typical of the high/soft spectral…

Astrophysics · Physics 2009-11-10 Aya Kubota , Kazuo Makishima

We present the first high-resolution, soft-X-ray spectrum of the prototypical Seyfert 2 galaxy, NGC 1068. This spectrum was obtained with the XMM-Newton Reflection Grating Spectrometer. Emission lines from H-like and He-like low-Z ions…

Supergiant fast X-ray transients are a new class of high mass X-ray binaries recently discovered with INTEGRAL. Hours long outbursts from these sources have been observed on numerous occasions at luminosities of ~1E36-1E37 erg/s, whereas…

Astrophysics · Physics 2009-11-13 E. Bozzo , L. Stella , G. Israel , M. Falanga , S. Campana

We present the results of a detailed analysis of RXTE observations which show an unusual state transition between high-soft and low-soft states in the microquasar GRS 1915+105. The RXTE pointed observations reveal that these events appeared…

Astrophysics · Physics 2007-05-23 S. Naik , A. R. Rao , Sandip K. Chakrabarti

We tabulate the luminosities of the soft-to-hard state transitions of all X-ray binaries for which there exist good X-ray flux measurements at the time of the transition, good distance estimates, and good mass estimates for the compact…

Astrophysics · Physics 2009-11-10 Thomas J. Maccarone

The Galactic microquasars GRS1915+105 and GRO J1655-40 were targets for dedicated monitoring programs with RXTE throughout 1996 and 1997. We review recent results with particular attention to the X-ray QPOs seen in these sources. We confirm…

Astrophysics · Physics 2009-09-25 R. A. Remillard , E. H. Morgan

We re-analyze archival Ginga data of the soft X-ray transient source GS 2023+338 covering the beginning of its May 1989 outburst. The source showed a number of rather unusual features: very high and apparently saturated luminosity, dramatic…

Astrophysics · Physics 2009-10-31 P. Zycki , C. Done , D. Smith

The well known black-hole X-ray binary transient XTE J1550-564 underwent an outburst during the spring of 2003 which was substantially underluminous in comparison to previous periods of peak activity in that source. In addition, our…

Astrophysics · Physics 2009-11-10 S. J. Sturner , C. R. Shrader

We present the analysis of several observations of the black hole binary GX 339--4 during its bright intermediate states from two different outbursts (2002 and 2004), as observed by RXTE/PCA. We perform a consistent study of its reflection…

High Energy Astrophysical Phenomena · Physics 2020-12-09 Navin Sridhar , Javier A. García , James F. Steiner , Riley M. T. Connors , Victoria Grinberg , Fiona A. Harrison

We report on two XMM-Newton observations of the low-mass X-ray binary X 1254-690. During an XMM-Newton observation of the low-mass X-ray binary in 2001 January a deep X-ray dip was seen while in a second observation one year later no dips…

Astrophysics · Physics 2009-11-10 L. Boirin , A. N. Parmar

We present the results of an archival 54 ks long Chandra observation of the peculiar source Cir X--1 during the phase passage 0.223-0.261. A comparative analysis of X-ray spectra, selected at different flux levels of the source, allows us…

Astrophysics · Physics 2009-06-23 A. D'Ai , R. Iaria , T. Di Salvo , G. Lavagetto , N. R. Robba

We present here the analysis of ultraviolet spectra from IUE and an X-ray spectrum from ROSAT PSPC observations of the X-ray weak, far-infrared loud AGN, PG 1126-041 (Mrk 1298). The first UV spectra taken in June 1992, simultaneously with…

Astrophysics · Physics 2016-08-30 T. G. Wang , W. Brinkmann , W. Wamsteker , W. Yuan , J. X. Wang

We report the discovery of a new, bright (V = 17 mag) AM Her system as the optical counterpart of the soft ROSAT All-Sky-Survey source RX J1846.9+5538 (= 1RXS J184659.4+553834). Optical photometric and spectroscopic follow-up observations…

Astrophysics · Physics 2009-11-07 R. Schwarz , J. Greiner , G. H. Tovmassian , S. V. Zharikov , W. Wenzel

AstroSat observed transient neutron star low-mass X-ray binary XTE J1701-462 for a total duration of $\sim$ 135 ks during its 2022 outburst. The source traced a complete `Z' shaped structure in the hardness intensity diagram (HID). The…

High Energy Astrophysical Phenomena · Physics 2025-04-02 Vivek K. Agrawal

Archival XMM-Newton data on the nearby Seyfert galaxy NGC 4051, taken in relatively high and low flux states, offer a unique opportunity to explore the complexity of its X-ray spectrum. We find the hard X-ray band to be significantly…

Astrophysics · Physics 2009-11-10 K. A. Pounds , J. N. Reeves , A. R. King , K. L. Page