activity
19962023
most citedX-ray Properties of Black-Hole Binaries

2.4k citations · 18.7k across the 158 of their papers we have counts for

collaborators
Showing astro-phShow all

71 papers · 1 filter

astro-ph2008★ 164 cited

A New Dynamical Model for the Black Hole Binary LMC X-1

Jerome A. Orosz, Danny Steeghs, Jeffrey E. McClintock +10

We present a dynamical model of the high mass X-ray binary LMC X-1 based on high-resolution optical spectroscopy and extensive optical and near-infrared photometry. From our new op…

astro-ph2007

Supplementary Information for "A 15.65 solar mass black hole in an eclipsing binary in the nearby spiral galaxy Messier 33"

Jerome A. Orosz, Jeffrey E. McClintock, Ramesh Narayan +8

This Supplementary Information provides details about the spectral extraction (crowding issues and the removal of nebular lines), a discussion about the distance to M33, a model fo…

astro-ph2007★ 257 cited

A 15.65 solar mass black hole in an eclipsing binary in the nearby spiral galaxy Messier 33

Jerome A. Orosz, Jeffrey E. McClintock, Ramesh Narayan +8

Stellar-mass black holes are discovered in X-ray emitting binary systems, where their mass can be determined from the dynamics of their companion stars. Models of stellar evolution…

astro-ph2007★ 8 cited

HST/NICMOS Observations of Fast Infrared Flickering in the Microquasar GRS 1915+105

Stephen S. Eikenberry, Shannon G. Patel, David M. Rothstein +3

We report infrared observations of the microquasar GRS 1915+105 using the NICMOS instrument of the Hubble Space Telescope during 9 visits in April-June 2003. During epochs of high…

astro-ph2007★ 150 cited

The 2003 Outburst of the X-ray Transient H 1743-322: Comparisons with the Black Hole Microquasar XTE J1550-564

Jeffrey E. McClintock, Ronald A. Remillard, Michael P. Rupen +4

The bright X-ray transient H 1743-322 was observed daily by the Rossi X-ray Timing Explorer (RXTE) during most of its 8-month outburst in 2003. We present a detailed spectral analy…

astro-ph2007★ 191 cited

Evaluating Spectral Models and the X-ray States of Neutron-Star X-ray Transients

Dacheng Lin, Ronald A. Remillard, Jeroen Homan

We propose a hybrid model to fit the X-ray spectra of atoll-type X-ray transients in the soft and hard states. This model uniquely produces luminosity tracks that are proportional…

astro-ph2006★ 34 cited

Joint H-alpha and X-ray Observations of Massive X-ray Binaries. I. The B-Supergiant System LS I +65 010 = 2S 0114+650

E. D. Grundstrom, J. L. Blair, D. R. Gies +8

We report on a three year spectroscopic monitoring program of the H-alpha emission in the massive X-ray binary LS I +65 010 = 2S 0114+650, which consists of a B-supergiant and a sl…

astro-ph2006★ 2.4k cited

X-ray Properties of Black-Hole Binaries

Ronald A. Remillard, Jeffrey E. McClintock

We review the properties and behavior X-ray binaries that contain an accreting black hole. The larger majority of such systems are X-ray transients, and many of them were observed…

astro-ph2006★ 586 cited

The Spin of the Near-Extreme Kerr Black Hole GRS 1915+105

Jeffrey E. McClintock, Rebecca Shafee, Ramesh Narayan +3

Based on a spectral analysis of the X-ray continuum that employs a fully relativistic accretion-disk model, we conclude that the compact primary of the binary X-ray source GRS 1915…

astro-ph2006★ 10 cited

XMM-Newton Discovery of the X-ray Transient XMMU J181227.8-181234 in the Galactic Plane

Edward M. Cackett, Rudy Wijnands, Ron Remillard

We report the discovery of an X-ray transient, observed in outburst with XMM-Newton on March 20, 2003, and with position 18h12m27.8s, -18 12 34 (J2000, approximate positional error…

astro-ph2005★ 30 cited

X-ray Spectral States and High-Frequency QPOs in Black Hole Binaries

R. A. Remillard

The high-frequency quasi-periodic oscillations in the X-ray emission of black hole binaries and candidates are briefly examined with respect to the question of X-ray states. We use…

astro-ph2005★ 32 cited

The Rates of type I X-ray Bursts from Transients Observed with RXTE: Evidence for Black Hole Event Horizons

Ronald A. Remillard, Dacheng Lin, Randall L. Cooper +1

We measure the rates of type I X-ray bursts, as a function of the bolometric luminosity, from a likely complete sample of 37 non-pulsing transients (1996-2004). Our goals are to te…

astro-ph2005★ 376 cited

Estimating the Spin of Stellar-Mass Black Holes via Spectral Fitting of the X-ray Continuum

Rebecca Shafee, Jeffrey E. McClintock, Ramesh Narayan +3

We fit X-ray spectral data in the thermal dominant or high soft state of two dynamically confirmed black holes, GRO J1655-40 and 4U 1543-47, and estimate the dimensionless spin par…

astro-ph2005

X-ray States of Black-Hole Binaries and Implications for the Mechanism of Steady Jets

R. A. Remillard

The three X-ray states of active accretion in black-hole binaries have been re-defined to focus attention on different physical elements that may contribute radiation: the accretio…

astro-ph2005★ 4 cited

X-ray States of Black Hole Binaries in Outburst

R. A. Remillard

A brief review is given for X-ray properties of black hole binary systems. Topics include the effort to re-define the three states of active accretion, potential applications for g…

astro-ph2004★ 13 cited

A Lack of Radio Emission from Neutron Star Low Mass X-ray Binaries

Michael P. Muno, Tomaso Belloni, Vivek Dhawan +3

We report strict upper limits to the radio luminosities of three neutron star low-mass X-ray binaries obtained with the Very Large Array while they were in hard X-ray states as obs…

astro-ph2004★ 75 cited

The X-ray Outburst of H1743-322: High-Frequency QPOs with a 3:2 Frequency Ratio

Ronald A. Remillard, Jeffrey E. McClintock, Jerome A. Orosz +1

We observed the 2003 X-ray outburst of H1743-322 in a series of 130 pointed observation with RXTE. We searched individual observations for high-frequency QPOs (HFQPOs) and found on…

astro-ph2004★ 122 cited

Orbital Parameters for the Black Hole Binary XTE J1650-500

Jerome A. Orosz, Jeffrey E. McClintock, Ronald A. Remillard +1

(Shortened) We present R-band photometry of the X-ray transient and candidate black hole binary XTE J1650-500 obtained between 2003 May and August with the 6.5m Clay Telescope. A t…

astro-ph2004★ 93 cited

The importance of discovering a 3:2 twin-peak QPO in a ULX or how to solve the puzzle of intermediate mass black holes

Marek A. Abramowicz, Wlodek Kluzniak, Jeffrey E. McClintock +1

Recently, twin-peak QPOs have been observed in a 3:2 ratio for three Galactic black-hole microquasars with frequencies that have been shown to scale as 1/M, as expected for general…

astro-ph2003★ 376 cited

Multiwavelength Observations of Strong Flares From the TeV-Blazar 1ES 1959+650

H. Krawczynski, S. B. Hughes, D. Horan +16

Following the detection of strong TeV gamma-ray flares from the BL Lac object 1ES 1959+650 with the Whipple 10 m Cherenkov telescope on May 16 and 17, 2002, we performed intensive…

astro-ph2003

Black Hole Binaries

Jeffrey E. McClintock, Ronald A. Remillard

We review the properties of 40 X-ray binaries that contain either a confirmed black hole or a black hole candidate. After discussing briefly the significance of these Galactic blac…

astro-ph2003★ 111 cited

Multiwavelength Spectrum of the Black Hole XTE J1118+480 in Quiescence

Jeffrey E. McClintock, Ramesh Narayan, Michael R. Garcia +3

We present an X-ray/UV/optical spectrum of the black hole primary in the X-ray nova XTE J1118+480 in quiescence at L_x = 4 x 10^{-9} of the Eddington luminosity. The Chandra, HST a…

astro-ph2003★ 10 cited

Mirax: A Brazilian X-Ray Astronomy Satellite Mission

J. Braga, R. Rothschild, J. Heise +9

We describe the ``Monitor e Imageador de Raios-X'' (MIRAX), an X-ray astronomy satellite mission proposed by the high energy astrophysics group at the National Institute for Space…

astro-ph2002★ 55 cited

Revealing the Focused Companion Wind in Cygnus X-1 with Chandra

J. M. Miller, P. Wojdowski, N. S. Schulz +5

We have analyzed a Chandra HETGS spectrum of the Galactic black hole Cygnus X-1, obtained at a source flux which is approximately twice that commonly observed in its persistent low…