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Articles: 2'506'133
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27 April 2024
 
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Results 1 to 20 of 403 for query "A. K. H. Kong". (0.01 sec.)

[    1    2    3    4    5    10    ]   Next

1.
Quasisoft X-Ray Sources: Unusual States of Stellar-Mass Objects, or Intermediate Mass Black Holes?
R. Di Stefano; F.A. Primini; A.K.H. Kong; T. Russo;
12 May 2004
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2.
Supersoft and Quasisoft X-Ray Sources in the Globular Clusters of NGC 4472: Are they candidates for intermediate-mass black holes?
R. Di Stefano; R. Friedman; A. Kundu; A.K.H. Kong;
15 Dec 2003
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3.
A "Combination Nova" Outburst in Z Andromedae: Nuclear Shell Burning Triggered by a Disk Instability
J. L. Sokoloski; S. J. Kenyon; B. R. Espey; Charles D. Keyes; S. R. McCandliss; A. K. H. Kong; J. P. Aufdenberg; A. V. Filippenko; W. Li; C. Brocksopp; Christian R. Kaiser; P. A. Charles; M. P. Rupen; R. P. S. Stone ( SAO; Trinity College Dublin; Dublin IAS; STScI; JHU; NOAO; U. C. Berkeley; MSSL; U. Southampton; SAAO; NRAO;
21 Sep 2005
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4.
MMT Observations of the Black Hole Candidate XTE J1118+480 near and in Quiescence
M. A. P. Torres; P. J. Callanan; M. R. Garcia; P. Zhao; S. Laycock; A. K. H. Kong;
26 May 2004   /  Astrophys.J. 612 (2004) 1026-1033
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5.
The X-ray source population of the globular cluster M15: Chandra high resolution imaging
D. C. Hannikainen; P. A. Charles; L. van Zyl; A. K. H. Kong; L. Homer; P. Hakala; T. Naylor; M. B. Davies;
22 Nov 2004   /  Mon.Not.Roy.Astron.Soc. 357 (2005) 325-332
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6.
XMM-Newton observations of the spiral galaxy M74 (NGC 628)
Roberto Soria; Albert K. H. Kong;
20 Mar 2002
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7.
X-ray Point Sources in the Sombrero Galaxy: Supersoft sources, the globular cluster/LMXB connection, and an overview
R. Di Stefano; A.K.H. Kong; M.L. VanDalfsen; W.E. Harris; S.S. Murray; K.M. Delain;
22 Jun 2003   /  Astrophys.J. 599 (2003) 1067-1081
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8.
Supersoft X-ray Sources in M31: I. A Chandra Survey and an Extension to Quasisoft Sources
R. Di Stefano; A.K.H. Kong; J. Greiner; F.A. Primini; M.R. Garcia; P. Barmby; P. Massey; P.W. Hodge; B.F. Williams; S.S. Murrary; S. Curry; T.A. Russo;
22 Jun 2003   /  Astrophys.J. 610 (2004) 247-260
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9.
A Luminous Recurrent Supersoft X-ray Source in NGC 300
A.K.H. Kong; R. Di Stefano;
28 Apr 2003   /  Astrophys.J. 590 (2003) L13-L16
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10.
Long-term X-ray variability and state transition of GX 339-4
A.K.H. Kong; P.A. Charles; E. Kuulkers; S. Kitamoto;
1 Oct 2001   /  Mon.Not.Roy.Astron.Soc. 329 (2002) 588
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11.
Bright X-Ray Sources in M31 Globular Clusters
R. Di Stefano; A.K.H. Kong; M.R. Garcia; P. Barmby; J. Greiner; S.S. Murray; F.A. Primini;
15 Jun 2001
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12.
X-ray/Optical/Radio Observations of a Resolved Supernova Remnant in NGC 6822
A.K.H. Kong; L.O. Sjouwerman; B.F. Williams;
18 Aug 2004
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13.
The Discovery of a Spatially-Resolved Supernova Remnant in M31 with Chandra
A.K.H. Kong; M.R. Garcia; F.A. Primini; S.S. Murray;
18 Oct 2002   /  Astrophys.J. 580 (2002) L125-L128
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14.
X-ray/Optical Bursts from GS 1826-24
A.K.H. Kong; L. Homer; E. Kuulkers; P.A. Charles; A.P. Smale;
29 Sep 1999
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15.
Luminous Supersoft X-Ray Sources in External Galaxies
R. Di Stefano; A.K.H. Kong;
9 Dec 2002   /  Astrophys.J. 592 (2003) 884-899
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16.
Chandra Studies of the X-ray Point Source Luminosity Functions of M31
A.K.H. Kong; R. Di Stefano; M.R. Garcia; J. Greiner;
4 Nov 2002
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17.
A detailed X-ray investigation of PSR J2021+4026 and $gamma$-Cygni supernova remnant
C. Y. Hui; K. A. Seo; L. C. C. Lin; R. H. H. Huang; C. P. Hu; J. H. K. Wu; L. Trepl; J. Takata; Y. Wang; Y. Chou; K. S. Cheng; A. K. H. Kong;
9 Nov 2014
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18.
Search for pulsed gamma-ray emission from globular cluster M28
J. H. K. Wu; C. Y. Hui; E. M. H. Wu; A. K. H. Kong; R. H. H. Huang; P. H. T. Tam; J. Takata; K. S. Cheng;
4 Feb 2013
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19.
The Discovery of Quasisoft and Supersoft Sources in External Galaxies
R. Di Stefano; A.K.H. Kong;
17 Nov 2003   /  Astrophys.J. 609 (2004) 710-727
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20.
Discovery of an unidentified Fermi object as a black widow-like millisecond pulsar
A. K. H. Kong; R. H. H. Huang; K. S. Cheng; J. Takata; Y. Yatsu; C. C. Cheung; D. Donato; L. C. C. Lin; J. Kataoka; Y. Takahashi; K. Maeda; C. Y. Hui; P. H. T. Tam;
17 Jan 2012
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