中文
相关论文

相关论文: An Anomalous Quiescent Stellar Mass Black Hole

200 篇论文

We report the result of a new Chandra observation of the black hole X-ray transient H 1705-250 in quiescence. H 1705-250 was barely detected in the new 50 ks Chandra observation. With 5 detected counts, we estimate the source quiescent…

高能天体物理现象 · 物理学 2015-06-11 Yi-Jung Yang , Albert K. H. Kong , David M. Russell , Fraser Lewis , Rudy Wijnands

The quiescent state is the dominant accretion mode for black holes on all mass scales. Our knowledge of the X-ray spectrum is limited due to the characteristic low luminosity in this state. Herein, we present an analysis of the sample of…

高能天体物理现象 · 物理学 2015-06-19 Mark T. Reynolds , Rubens C. Reis , Jon M. Miller , Edward M. Cackett , Nathalie Degenaar

Using the Chandra X-ray Observatory, we have detected the black hole transients V4641 Sgr and XTE J1859+226 in their low luminosity, quiescent states. The 0.3-8 keV luminosities are (4.0^(+3.3)_(-2.4))E31 (d/7 kpc)^2 erg/s and…

GRS 1915$+$105 is a stellar-mass black hole that is well known for exhibiting at least 12 distinct classes of X-ray variability and correlated multi-wavelength behavior. Despite such extraordinary variability, GRS 1915$+$105 remained one of…

高能天体物理现象 · 物理学 2021-03-10 Mayura Balakrishnan , J. M. Miller , M. T. Reynolds , E. Kammoun , A. Zoghbi , B. E. Tetarenko

The Galactic black hole X-ray binary XTE J1650-500 entered a quiescent regime following the decline from the 2001-2002 outburst that led to its discovery. Here we report on the first detection of its quiescent counterpart in a 36 ks…

天体物理学 · 物理学 2009-11-13 Elena Gallo , Jeroen Homan , Peter Jonker , John Tomsick

We present the results of a NuSTAR study of the dynamically confirmed stellar-mass black hole GS 1354-645. The source was observed during its 2015 "hard" state outburst; we concentrate on spectra from two relatively bright phases. In the…

We report the results of observations of the black hole binaries XTE J1550-564 and H 1743-322 in their quiescent state using the Chandra X-ray Observatory. Both sources are detected at their faintest level of X-ray emission ever observed…

天体物理学 · 物理学 2009-11-13 S. Corbel , J. A. Tomsick , P. Kaaret

We report on XMM-Newton observations of GRO J1655-40 and GRS 1009-45, which are two black hole X-ray transients currently in their quiescent phase. GRO J1655-40 was detected with a 0.5 - 10 keV luminosity of 5.9 10^{31} erg/s. This…

天体物理学 · 物理学 2009-11-07 J. -M. Hameury , D. Barret , J. -P. Lasota , J. E. McClintock , K. Menou , C. Motch , J. -F. Olive , N. Webb

Little is known about the properties of the accretion flows and jets of the lowest-luminosity quiescent black holes. We report new, strictly simultaneous radio and X-ray observations of the nearby stellar-mass black hole X-ray binary GS…

高能天体物理现象 · 物理学 2020-02-05 J. Rodriguez , R. Urquhart , R. M. Plotkin , T. Panurach , L. Chomiuk , J. Strader , J. C. A. Miller-Jones , E. Gallo , G. R. Sivakoff

We present XMM observations of the black hole X-ray nova V404 Cygni in quiescence. Its quiescent spectrum can be best fitted by a simple power-law with slope 2. The spectra are consistent with that expected for the advection-dominated…

天体物理学 · 物理学 2011-02-11 C. K. Bradley , R. I. Hynes , A. K. H. Kong , C. A. Haswell , J. Casares , E. Gallo

The Galactic transient black hole GS 1354-64 recently showed a new outburst, which has been continuously monitored by {\it MAXI}, {\it NuSTAR} and {\it Insight-HXMT} missions. The ongoing $2025-26$ outburst shows a slow-rise with an unusual…

高能天体物理现象 · 物理学 2026-05-28 Dipak Debnath , Hsiang-Kuang Chang , Subham Srimani , Anuj Nandi

An observation of the gravitationally lensed system 2016+112 with the Chandra X-ray Observatory has resolved a mystery regarding the proposed presence of a dark matter object in the lens plane of this system. The Chandra ACIS observation…

天体物理学 · 物理学 2009-11-06 G. Chartas , M. Bautz , G. Garmire , C. Jones , D. P. Schneider

We present Chandra observations of black hole X-ray novae V404 Cyg, A0620-00, GRO J1655-40 and XTE J1550-564 in quiescence. Their quiescent spectra can be well fitted by a power-law model with slope $\alpha \sim 2$. While a coronal…

天体物理学 · 物理学 2009-11-07 A. K. H. Kong , J. E. McClintock , M. R. Garcia , S. S. Murray , D. Barret

Observations of V404 Cyg performed with the Westerbork Synthesis Radio Telescope at four frequencies, over the interval 1.4-8.4 GHz, have provided us with the first broadband radio spectrum of a `quiescent' stellar mass black hole. The…

天体物理学 · 物理学 2009-11-10 Elena Gallo , Rob Fender , Rob Hynes

The results of photometric CCD monitoring and spectral observations of the black hole binary and microquasar V4641 Sgr in the quiet state are presented. The ellipsoidal light curve with large amplitude of 0.36^m in R band suggests the…

天体物理学 · 物理学 2007-05-23 V. P. Goranskij , E. A. Barsukova , A. N. Burenkov , D. N. Monin

Since its outburst in 1997 GS 135-64 stayed in quiescence. In June 2015 renewed activity of GS 1354-64 was observed. Based on our analysis of energy spectra and timing properties obtained from Swift/XRT monitoring data we found that GS…

高能天体物理现象 · 物理学 2016-05-04 H. Stiele , A. K. H. Kong

We report a characterization of an X-ray-detected quiescent galaxy at $z=2.09$, named COS-XQG1, using JWST/NIRCam and NIRSpec data. This galaxy is detected in Chandra imaging, suggesting the presence of an AGN with a high black hole…

We present coordinated multiwavelength observations of the high Galactic latitude (b=+50 deg) black hole X-ray binary (XRB) J1357.2-0933 in quiescence. Our broadband spectrum includes strictly simultaneous radio and X-ray observations, and…

We present new Chandra X-ray observations of the transient black hole X-ray binary MAXI J1659-152 in quiescence. These observations were made more than one year after the end of the source's 2010-2011 outburst. We detect the source at a…

We present a 45 ks Chandra observation of the quasar ULAS J1342+0928 at z=7.54. We detect 14.0^{+4.8}_{-3.7} counts from the quasar in the observed-frame energy range 0.5-7.0 keV (6-sigma detection), representing the most distant…

‹ 上一页 1 2 3 10 下一页 ›