A Chandra X-ray observation of the globular cluster Terzan 1
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E. Cackett | R. Wijnands | P. Jonker | D. Pooley | J. Grindlay | W. Lewin | C. Heinke | P. Edmonds | J. Miller | P. G. Jonker | Jon M. Miller | P. Jonker
[1] P. S. Bunclark,et al. Astronomical Data Analysis Software and Systems , 2008 .
[2] L. A. Antonelli,et al. Interacting Binaries: Accretion, Evolution, Outcomes , 2005 .
[3] K. Dooley,et al. Formation of Ultracompact X-Ray Binaries in Dense Star Clusters , 2005, astro-ph/0501617.
[4] E. Cackett,et al. X-Ray Variability during the Quiescent State of the Neutron Star X-Ray Transient in the Globular Cluster NGC 6440 , 2004, astro-ph/0407448.
[5] Michael R. Garcia,et al. Optical and X-ray observations of the neutron star soft X-ray transient XTE J1709–267 , 2004, astro-ph/0406208.
[6] E. Feigelson,et al. The Spectra and Variability of X-Ray Sources in a Deep Chandra Observation of the Galactic Center , 2004, astro-ph/0403463.
[7] S. Murray,et al. A Chandra X-Ray Study of the Globular Cluster M80 , 2003, astro-ph/0305443.
[8] J. Grindlay,et al. Analysis of the Quiescent Low-Mass X-Ray Binary Population in Galactic Globular Clusters , 2003, astro-ph/0305445.
[9] S. Anderson,et al. Dynamical Formation of Close Binary Systems in Globular Clusters , 2003, astro-ph/0305003.
[10] J. E. Grindlay,et al. A Chandra X-Ray Study of the Dense Globular Cluster Terzan 5 , 2003, astro-ph/0303141.
[11] J. Munn,et al. The USNO-B Catalog , 2002, astro-ph/0210694.
[12] R. Wijnands,et al. A Chandra Observation of the Globular Cluster Terzan 1: The Neutron Star X-Ray Transient X1732–304 in Quiescence , 2001, astro-ph/0111337.
[13] V. Kaspi,et al. ACCEPTED BY THE Astrophysical Journal Preprint typeset using L ATEX style emulateapj v. 14/09/00 CHANDRA OBSERVATION OF THE GLOBULAR CLUSTER NGC 6440 AND THE NATURE OF CLUSTER X-RAY LUMINOSITY FUNCTIONS , 2002 .
[14] S. Anderson,et al. Optical Identification of Multiple Faint X-Ray Sources in the Globular Cluster NGC 6752: Evidence for Numerous Cataclysmic Variables , 2001, astro-ph/0110192.
[15] D. Lamb,et al. A Wavelet-Based Algorithm for the Spatial Analysis of Poisson Data , 2001, astro-ph/0108429.
[16] J. Grindlay,et al. Chandra Exposes the Core-collapsed Globular Cluster NGC 6397 , 2001, astro-ph/0108265.
[17] R. Wijnands,et al. A Chandra Observation of the Long-Duration X-Ray Transient KS 1731–260 in Quiescence: Too Cold a Neutron Star? , 2001, astro-ph/0107380.
[18] Chris Biemesderfer,et al. Astronomical Data Analysis Software and Systems X , 2001 .
[19] S. Murray,et al. High-Resolution X-ray Imaging of a Globular Cluster Core: Compact Binaries in 47Tuc , 2001, Science.
[20] J. Lasota. The disc instability model of dwarf novae and low-mass X-ray binary transients , 2001, astro-ph/0102072.
[21] M. Colpi,et al. Charting the Temperature of the Hot Neutron Star in a Soft X-Ray Transient , 2000, astro-ph/0010572.
[22] K. Menou,et al. The Quiescent Emission Spectrum of Centaurus X-4 and Other X-Ray Transients Containing Neutron Stars , 2000, astro-ph/0010430.
[23] Margarita Karovska,et al. Initial performance of the aspect system on the Chandra Observatory: postfacto aspect reconstruction , 2000, Astronomical Telescopes and Instrumentation.
[24] S. Borgani,et al. First Results from the X-Ray and Optical Survey of the Chandra Deep Field South , 2000, astro-ph/0007240.
[25] Bernd Aschenbach,et al. X-Ray Optics, Instruments, and Missions III , 2000 .
[26] L. Stella,et al. On the Bolometric Quiescent Luminosity and Luminosity Swing of Black Hole Candidate and Neutron Star Low-Mass X-Ray Transients , 2000, astro-ph/0005118.
[27] F. Ochsenbein,et al. The VizieR database of astronomical catalogues , 2000, astro-ph/0002122.
[28] L. Bildsten,et al. Crustal Heating and Quiescent Emission from Transiently Accreting Neutron Stars , 1998, astro-ph/9807179.
[29] William E. Harris,et al. A Catalog of Parameters for Globular Clusters in the Milky Way , 1996 .
[30] N. Khavenson,et al. SIGMA Detection of Hard X-Ray Emission from the Terzan 1 Globular Cluster , 1996 .
[31] M. Colpi,et al. Do quiescent soft X-ray transients contain millisecond radio pulsars? , 1994 .
[32] S. Campana,et al. The neutron stars of Soft X–ray Transients , 1993, astro-ph/9805079.
[33] M. Turner,et al. A survey of the galactic plane with EXOSAT , 1988 .
[34] G. Skinner,et al. Hard X-ray images of the galactic centre , 1987, Nature.
[35] K. Makishima,et al. X-ray burst sources near the galactic center and their burst peak luminosities. , 1981 .
[36] K. Koyama,et al. Discovery of two new X-ray burst sources in the globular clusters Terzan 1 and Terzan 5 , 1981 .
[37] W. Cash,et al. Parameter estimation in astronomy through application of the likelihood ratio. [satellite data analysis techniques , 1979 .
[38] Carlos E. C. J. Gabriel,et al. Astronomical Data Analysis Software and Systems Xv , 2022 .
[40] S. Djorgovski,et al. New horizons in globular cluster astronomy : proceedings of a conference held at Università di Padova, Padova, Italy 24-28 June, 2002 , 2003 .
[41] M. Perrin,et al. Metallicity and radial velocity of the second parameter globular cluster Terzan 1 in the galactic bulge , 2002 .
[42] Scott Trager,et al. Catalogue of Galactic globular-cluster surface-brightness profiles , 1995 .
[43] R. Sunyaev,et al. The X-ray burster SLX1732-304 in the globular cluster Terzan-1: Observations with the ART-P telescope on board the Granat observatory☆ , 1995 .
[44] Georges Meylan,et al. Structure and dynamics of globular clusters , 1993 .
[45] D. Helfand,et al. The Origin and Evolution of Neutron Stars , 1987 .
[46] J. Grindlay. X-Ray Sources in Globular Clusters , 1981 .