Zobrazeno 1 - 10
of 48
pro vyhledávání: '"Robert E. Rutledge"'
Autor:
Dale A. Frail, Brian P. Schmidt, Daniel E. Holz, Scott S. Sheppard, S. J. Bell Burnell, Lennox L. Cowie, P. B. Cameron, Derek B. Fox, Robert E. Rutledge, Antonino Cucchiara, Arne Rau, Katherine C. Roth, I. M. Hook, Michael A. Dopita, Edo Berger, Shrinivas R. Kulkarni, Bryan E. Penprase, Stephen Bradley Cenko, Ehud Nakar, Antoinette Songaila, Eran O. Ofek, Paul A. Price, Bruce A. Peterson, Alicia M. Soderberg, Avishay Gal-Yam, Ph. Podsiadlowski
The redshift distribution of the short-duration GRBs is a crucial, but currently fragmentary, clue to the nature of their progenitors. Here we present optical observations of nine short GRBs obtained with Gemini, Magellan, and the Hubble Space Telesc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b13e69088e381faa2ea5e0f999ab58cd
https://doi.org/10.1086/518762
https://doi.org/10.1086/518762
Publikováno v:
The Astrophysical Journal. 705:391-397
We report the results of a 30 ks Chandra ACIS-S observation of the isolated compact object 1RXS J141256.0+792204 (Calvera). The X-ray spectrum is adequately described by an absorbed neutron star hydrogen atmosphere model with an effective temperature
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::784b78bf044410aa450abce8754d5c57
https://doi.org/10.1088/0004-637x/705/1/391
https://doi.org/10.1088/0004-637x/705/1/391
Autor:
Sebastien Guillot, Edward F. Brown, Vyacheslav E. Zavlin, Robert E. Rutledge, George G. Pavlov
Publikováno v:
The Astrophysical Journal. 699:1418-1422
This paper presents the analysis of candidate quiescent low mass xray binarie (qLMXBs) observed during a short Chandra/ACIS observation of the globular cluster (GC) NGC 6304. Two out of the three candidate qLMXBs of this cluster, XMMU 171433-292747 a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b60edcaba65a5c6b55d943d2531155f2
https://doi.org/10.1088/0004-637x/699/2/1418
https://doi.org/10.1088/0004-637x/699/2/1418
Autor:
Stephen S. Murray, Ismaël Cognard, S. R. Kulkarni, Robert E. Rutledge, Derek Fox, Bryan A. Jacoby, D. C. Backer
Publikováno v:
The Astrophysical Journal. 613:522-531
We perform absolute timing of PSR B1821-24 in M28, using a 50 ksec observation with Chandra/HRC-S. We have obtained the highest signal-to-noise X-ray pulsed lightcurve of this source to date, detecting two X-ray pulses, as well as significant non-pul
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3cc130a1050e6a7626c8e9299fd8197e
https://doi.org/10.1086/380299
https://doi.org/10.1086/380299
Publikováno v:
The Astrophysical Journal. 607:90-102
We describe new optical images and spectra of POX 52, a dwarf galaxy with an active nucleus that was originally detected in the POX objective-prism survey. While POX 52 was originally thought to be a Seyfert 2 galaxy, the new data reveal an emission-
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a4ecf9f9f3d2947392323f7a933fbb6e
https://doi.org/10.1086/383302
https://doi.org/10.1086/383302
Publikováno v:
The Astrophysical Journal. 578:405-412
Using the Chandra/ACIS-I detector, we have identified an X-ray source (CXOU 132619.7-472910.8) in the globular cluster NGC 5139 with a thermal spectrum identical to that observed from transiently accreting neutron stars in quiescence. The absence of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::57cacef8cd9177b7645fbd4f938c34a4
https://doi.org/10.1086/342306
https://doi.org/10.1086/342306
Publikováno v:
The Astrophysical Journal. 577:346-358
We obtained four Chandra/ACIS-S observations beginning two weeks after the end of the November 2000 outburst of the neutron star (NS) transient Aql X-1. Over the five month span in quiescence, the X-ray spectra are consistent with thermal emission fr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4dc294417d18b9097f2a2fab30064e3c
https://doi.org/10.1086/342155
https://doi.org/10.1086/342155
Autor:
Sebastien Guillot, Robert E. Rutledge
Neutrons stars are unique laboratories to discriminate between the various proposed equations of state of matter at and above nuclear density. One sub-class of neutron stars - those inside quiescent low-mass X-ray binaries (qLMXBs) - produce a therma
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ef40dc7984e6884cddbb43af4c1b477f
Autor:
Robert E. Rutledge, Greg Ushomirsky
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 325:1157-1166
Transiently accreting neutron stars in quiescence (Lx
Comment: 12 pages, 5 figures, submitted to MNRAS
Comment: 12 pages, 5 figures, submitted to MNRAS
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9443ec4f1388c84caffd028632f68942
https://doi.org/10.1046/j.1365-8711.2001.04515.x
https://doi.org/10.1046/j.1365-8711.2001.04515.x
Autor:
R. Guerriero, Derek Fox, Walter H. G. Lewin, Tadayasu Dotani, Edward H. Morgan, Jon M. Miller, Herman L. Marshall, M. van der Klis, Robert E. Rutledge, Lars Bildsten
Publikováno v:
The Astronomical Journal. 122:21-25
We present observations of the Rapid Burster (RB, also known as MXB 1730-335) using the Chandra High Energy Transmission Grating Spectrometer. The average interval between type II (accretion) bursts was about 40 s. There was one type I (thermonuclear
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::fa7296af7e540e0a06f302e6e45faa51
https://doi.org/10.1086/321142
https://doi.org/10.1086/321142