Search Results - "Heinke, C. O."
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Strong disk winds traced throughout outbursts in black-hole X-ray binaries
Published in Nature (London) (01-02-2018)“…Analysis of the light curves of outbursts in black-hole X-ray binaries suggests that throughout the accretion process mass is lost from the accretion disks…”
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Constraining the mass and radius of neutron stars in globular clusters
Published in Monthly notices of the Royal Astronomical Society (01-05-2018)“…Abstract We analyse observations of eight quiescent low-mass X-ray binaries in globular clusters and combine them to determine the neutron star mass–radius…”
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3
Deep radio imaging of 47 Tuc identifies the peculiar X-ray source X9 as a new black hole candidate
Published in Monthly notices of the Royal Astronomical Society (11-11-2015)“…We report the detection of steady radio emission from the known X-ray source X9 in the globular cluster 47 Tuc. With a double-peaked C iv emission line in its…”
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Formation and evolution of compact binaries in globular clusters – II. Binaries with neutron stars
Published in Monthly notices of the Royal Astronomical Society (01-05-2008)“…In this paper, the second of a series, we study the stellar dynamical and evolutionary processes leading to the formation of compact binaries containing…”
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5
New cataclysmic variables and other exotic binaries in the globular cluster 47 Tucanae
Published in Monthly notices of the Royal Astronomical Society (21-04-2018)“…Abstract We present 22 new (+3 confirmed) cataclysmic variables (CVs) in the non-core-collapsed globular cluster 47 Tucanae (47 Tuc). The total number of CVs…”
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Further Constraints on Thermal Quiescent X-Ray Emission from SAX J1808.4-3658
Published in The Astrophysical journal (01-02-2009)“…We observed SAX J1808.4-3658 (1808), the first accreting millisecond pulsar, in deep quiescence with XMM-Newton and (near simultaneously) Gemini-South. The…”
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THE FIRST LOW-MASS BLACK HOLE X-RAY BINARY IDENTIFIED IN QUIESCENCE OUTSIDE OF A GLOBULAR CLUSTER
Published in The Astrophysical journal (01-07-2016)“…ABSTRACT The observed relation between the X-ray and radio properties of low-luminosity accreting black holes (BHs) has enabled the identification of multiple…”
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The Swift bulge survey: motivation, strategy, and first X-ray results
Published in Monthly notices of the Royal Astronomical Society (01-02-2021)“…ABSTRACT Very faint X-ray transients (VFXTs) are X-ray transients with peak X-ray luminosities (LX) of L$_X \lesssim 10^{36}$ erg s−1, which are not well…”
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Formation of Black Hole X-ray Binaries in Globular Clusters
Published in The Astrophysical journal (10-07-2010)“…Inspired by the recent identification in extragalactic globular clusters of the first candidate black hole-white dwarf (BH-WD) X-ray binaries, where the…”
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Enhanced optical activity 12 d before X-ray activity, and a 4 d X-ray delay during outburst rise, in a low-mass X-ray binary
Published in Monthly notices of the Royal Astronomical Society (01-11-2020)“…ABSTRACT X-ray transients, such as accreting neutron stars, periodically undergo outbursts, thought to be caused by a thermal-viscous instability in the…”
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11
Flaring Activity of Sagittarius A at 43 and 22 GHz: Evidence for Expanding Hot Plasma
Published in The Astrophysical journal (10-10-2006)“…We have carried out Very Large Array (VLA) continuum observations to study the variability of Sgr A* at 43 GHz (l = 7 mm) and 22 GHz (l = 13 mm). A low level…”
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12
Neutron star crust cooling in the Terzan 5 X-ray transient Swift J174805.3–244637
Published in Monthly notices of the Royal Astronomical Society (01-08-2015)“…When neutron stars reside in transient X-ray binaries, their crustal layers become heated during accretion outbursts and subsequently cool in quiescence…”
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A Swift study of long-term changes in the X-ray flaring properties of Sagittarius A
Published in Monthly notices of the Royal Astronomical Society (01-02-2022)“…ABSTRACT The radiative counterpart of the supermassive black hole at the Galactic Centre, Sagittarius A*, displays flaring emission in the X-ray band atop a…”
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14
Constraints on Thermal X-Ray Radiation from SAX J1808.4–3658 and Implications for Neutron Star Neutrino Emission
Published in The Astrophysical journal (10-05-2007)“…Thermal X-ray radiation from neutron star soft X-ray transients in quiescence provides the strongest constraints on the cooling rates of neutron stars and thus…”
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15
A superburst candidate in EXO 1745-248 as a challenge to thermonuclear ignition models
Published in Monthly notices of the Royal Astronomical Society (21-10-2012)“…Abstract We report on Chandra, Rossi X-ray Timing Explorer (RXTE), Swift/Burst Alert Telescope (BAT) and MAXI observations of an X-ray flare of ∼1 d and…”
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A Deep Chandra Survey of the Globular Cluster 47 Tucanae: Catalog of Point Sources
Published in The Astrophysical journal (01-06-2005)“…We have detected 300 X-ray sources within the half-mass radius (2.'79) of the globular cluster 47 Tucanae in a deep (281 ks) Chandra exposure. We perform…”
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Discovery of a Second Transient Low-Mass X-ray Binary in the Globular Cluster Ngc 6440
Published in The Astrophysical journal (01-05-2010)“…We have discovered a new transient low-mass X-ray binary, NGC 6440 X-2, with Chandra/ACIS, RXTE/PCA, and Swift/XRT observations of the globular cluster NGC…”
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18
Formation and evolution of compact binaries in globular clusters – I. Binaries with white dwarfs
Published in Monthly notices of the Royal Astronomical Society (01-11-2006)“…In this paper, the first of a series, we study the stellar dynamical and evolutionary processes leading to the formation of compact binaries containing white…”
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A Radio Frequency Study of the Accreting Millisecond X-ray Pulsar, IGR J16597-3704, in the Globular Cluster NGC 6256
Published in The Astrophysical journal (20-02-2018)“…We present Karl G. Jansky Very Large Array radio frequency observations of the new accreting millisecond X-ray pulsar (AMXP), IGR J16597−3704, located in the…”
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Extreme quiescent variability of the transient neutron star low-mass X-ray binary EXO 1745−248 in Terzan 5
Published in Monthly notices of the Royal Astronomical Society (11-09-2018)Get full text
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