SIGMA observation of hard X-ray emission from the ultrasoft X-ray transient Triangulum Australe X-1 (A1524 - 62)

Barret, D.; Roques, J. P.; Mandrou, P.; Bouchet, L.; Lebrun, F.; Goldwurm, A.; Laurent, P.; Paul, J.; Sunyaev, R.; Churazov, E.; Gilfanov, M.; Diachkov, A.; Kavenson, N.; Novikov, B.; Chulkov, I.; Kuznetsov, A.

doi:10.1086/186415

Cited by 20 publications

(6 citation statements)

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“… 1 Lewin, Clark & Smith (1968); 2 Li, Sprott & Clark (1976); 3 Matilsky et al (1972); 4 Kitamoto et al (1984); 5 Kaluzienski et al (1975); 6 Ricketts, Pounds & Turner (1975); 7 Kuulkers et al (1999); 8 Watson, Ricketts & Griffiths (1978); 9 Wilson & Rothschild (1983); 10 Tanaka & Lewin (1995); 11 Parmer et al (1993); 12 Ball et al (1995); 13 Ebisawa et al (1994); 14 Lapshov, Sazonov & Sunyaev (1993); 15 Harmon et al (1995); 16 Churazov et al (1994); 17 Vargas et al (1997); 18 Borozdin, Alexandrovich & Sunyaev (1996); 19 Hjellming et al (1996a); 20 Parmar et al (1997); 21 Hjellming et al (1999); 22 Smith, Levine & Wood (1998); 23 Harmon et al (1998); 24 Hjellming et al (1998); 25 Hannikainen et al (2001); 26 Vasiliev, Trudolyubov & Revnivtsev (2000); 27 this paper; 28 Hjellming et al (2000); 29 Barret et al (1992); 30 Harmon et al (1992b); 31 Shrader et al (1994); 32 Callanan et al (1995); 33 Revnivtsev et al (1998); 34 Hjellming et al (1996b); 35 Brocksopp et al (2001); 36 Wilson & McCollough (2000). …”

Section: Discussion and Comparison With Other Sourcesmentioning

confidence: 99%

Initial low/hard state, multiple jet ejections and X-ray/radio correlations during the outburst of XTE J1859+226

Brocksopp

Fender

McCollough

et al. 2002

Monthly Notices of the Royal Astronomical Society

102

141

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We have studied the 1999 soft X‐ray transient outburst of XTE J1859+226 at radio and X‐ray wavelengths. The event was characterized by strong variability in the disc, corona and jet – in particular, a number of radio flares (ejections) took place and seemed well‐correlated with hard X‐ray events. Apparently unusual for the canonical‘soft’ X‐ray transient, there was an initial period of low/hard state behaviour during the rise from quiescence but prior to the peak of the main outburst – we show that not only could this initial low/hard state be a ubiquitous feature of soft X‐ray transient outbursts, but also it could be extremely important in our study of outburst mechanisms.

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Section: Discussion and Comparison With Other Sourcesmentioning

confidence: 99%

Initial low/hard state, multiple jet ejections and X-ray/radio correlations during the outburst of XTE J1859+226

Brocksopp

Fender

McCollough

et al. 2002

Monthly Notices of the Royal Astronomical Society

102

141

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“…TrA showed another outburst in 1990 (Barret et al 1992). (29) 1H J1659-487 (GX 339-4) is a quasi persistent source.…”

Section: Kymentioning

confidence: 99%

BlackCAT: A catalogue of stellar-mass black holes in X-ray transients

Corral-Santana

Casares

Muñoz‐Darias

et al. 2016

A&A

426

346

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Aims. During the last ∼50 years, the population of black hole candidates in X-ray binaries has increased considerably, with 59 Galactic objects being detected in transient low-mass X-ray binaries, as well as a few in persistent systems (including ∼5 extragalactic binaries). Methods. We collect near-infrared, optical, and X-ray information spread over hundreds of references to study the population of black holes in X-ray transients as a whole.Results. We present the most updated catalogue of black hole transients. This contains X-ray, optical, and near-infrared observations, together with their astrometric and dynamical properties. The catalogue provides new and useful information in both statistical and observational parameters and provides a thorough and complete overview of the black hole population in the Milky Way. Analysing the distances and spatial distribution of the observed systems, we estimate a total population of ∼1300 Galactic black hole transients. This means that we have only discovered less than ∼5% of the total Galactic distribution.

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“…(o 3"): [128]; X-ray outburst in 1977: [786]; ultra-soft X-ray spectrum, BHC: [57,1410]; X-ray obs. : [60]; hard component in quiescent X-ray spectrum: [57]; optical outburst: [1124]; V quiesc >21: [1124] Pos. (o < 1"): [128]; X-ray obs.…”

Section: Conclusion and Remarksmentioning

confidence: 99%

A catalogue of low-mass X-ray binaries in the Galaxy, LMC, and SMC (Fourth edition)

Liu

Paradijs

Heuvel

2007

A&A

376

366

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We present a new edition of the catalogue of the low-mass X-ray binaries in the Galaxy and the Magellanic Clouds. The catalogue contains source name(s), coordinates, finding chart, X-ray luminosity, system parameters, and stellar parameters of the components and other characteristic properties of 187 low-mass X-ray binaries, together with a comprehensive selection of the relevant literature. The aim of this catalogue is to provide the reader with some basic information on the X-ray sources and their counterparts in other wavelength ranges (γ-rays, UV, optical, IR, and radio). Some sources, however, are only tentatively identified as low-mass X-ray binaries on the basis of their X-ray properties similar to the known low-mass X-ray binaries. Further identification in other wavelength bands is needed to finally determine the nature of these sources. In cases where there is some doubt about the low-mass nature of the X-ray binary this is mentioned. Literature published before 1 October 2006 has, as far as possible, been taken into account.

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SIGMA observation of hard X-ray emission from the ultrasoft X-ray transient Triangulum Australe X-1 (A1524 - 62)

Cited by 20 publications

References 0 publications

Initial low/hard state, multiple jet ejections and X-ray/radio correlations during the outburst of XTE J1859+226

Initial low/hard state, multiple jet ejections and X-ray/radio correlations during the outburst of XTE J1859+226

BlackCAT: A catalogue of stellar-mass black holes in X-ray transients

A catalogue of low-mass X-ray binaries in the Galaxy, LMC, and SMC (Fourth edition)

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