RX J004732.9-251748 , the SIMBAD biblio

RX J004732.9-251748 , the SIMBAD biblio (35 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST15:22:58

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
1984ApJ...286..491F 2 12 137 The complex X-emission of NGC 253. FABBIANO G. and TRINCHIERI G.
1988ApJ...330..672F 3 10 155 X-ray spectra and large-scale features of two starburst galaxies: NGC 253 and M 82. FABBIANO G.
1999A&A...342..101V 87 30 X-ray observations of the starburst galaxy NGC 253. I. Point sources in the bulge, disk and halo. VOGLER A. and PIETSCH W.
2000A&A...360...24P 31 57 X-ray observations of the starburst galaxy NGC 253. II. Extended emission from hot gas in the nuclear area, disk, and halo. PIETSCH W., VOGLER A., KLEIN U., et al.
2000MNRAS.312..689F 1 8 31 A multiwavelength view at the heart of the superwind in NGC253. FORBES D.A., POLEHAMPTON E., STEVENS I.R., et al.
2001A&A...365L.174P 2 12 77 XMM-Newton observations of NGC 253: Resolving the emission components in the disk and nuclear area. PIETSCH W., ROBERTS T.P., SAKO M., et al.
2003A&A...402..457P 11 8 RX J004717.4-251811: The first eclipsing X-ray binary outside the Local Group. PIETSCH W., HABERL F. and VOGLER A.
2003MNRAS.344..134H viz 88 36 Ultraluminous X-ray source populations in normal galaxies: a preliminary survey with Chandra. HUMPHREY P.J., FABBIANO G., ELVIS M., et al.
2004ApJ...602..231C viz 15       D               1486 200 Old and young X-ray point source populations in nearby galaxies. COLBERT E.J.M., HECKMAN T.M., PTAK A.F., et al.
2005A&A...429.1125L viz 339 66 A catalogue of ultraluminous X-ray sources in external galaxies. LIU Q.Z. and MIRABEL I.F.
2005ApJS..157...59L viz 840 130 Ultraluminous X-ray sources in nearby galaxies from ROSAT high resolution imager observations I. Data analysis. LIU J.-F. and BREGMAN J.N.
2006ApJ...649..730W viz 15       D               147 115 XMM-Newton archival study of the ultraluminous X-ray population in nearby galaxies. WINTER L.M., MUSHOTZKY R.F. and REYNOLDS C.S.
2007A&A...467..979B 148           X C       3 7 17 High-resolution X-ray spectroscopy and imaging of the nuclear outflow of the starburst galaxy NGC 253. BAUER M., PIETSCH W., TRINCHIERI G., et al.
2008ApJ...679.1405H 14 18 Detailed atmosphere model fits to disk-dominated ULX spectra. HUI Y. and KROLIK J.H.
2008MNRAS.388..849B viz 112           X   F     2 8 5 A multi-coloured survey of NGC253 with XMM-Newton: testing the methods used for creating luminosity functions from low-count data. BARNARD R., SHAW GREENING L. and KOLB U.
2008ApJ...687..471B viz 15       D               2 117 49 Testing the paradigm that ultraluminous X-ray sources as a class represent accreting intermediate-mass black holes. BERGHEA C.T., WEAVER K.A., COLBERT E.J.M., et al.
2009MNRAS.398.1450K 579       D     X C F     14 24 111 Spectral variability of ultraluminous X-ray sources. KAJAVA J.J.E. and POUTANEN J.
2009MNRAS.397.1061H 241       D     X C F     5 20 75 A systematic study of variability in a sample of ultraluminous X-ray sources. HEIL L.M., VAUGHAN S. and ROBERTS T.P.
2010ApJ...716..181J 38           X         1 12 11 Transition to the disk dominant state of a new ultraluminous X-ray source in M82. JIN J., FENG H. and KAARET P.
2011A&A...526A.132G 15       D               2 23 21 The scaling of X-ray variability with luminosity in ultra-luminous X-ray sources. GONZALEZ-MARTIN O., PAPADAKIS I., REIG P., et al.
2011ApJ...737...87J 76             C       1 91 13 XMM-Newton observations of NGC 247: X-ray population and a supersoft ultraluminous X-ray source. JIN J., FENG H., KAARET P., et al.
2011MNRAS.416.1844W viz 15       D               4 256 134 2XMM ultraluminous X-ray source candidates in nearby galaxies. WALTON D.J., ROBERTS T.P., MATEOS S., et al.
2012ApJ...756...27L viz 15       D               1 4347 64 Classification of X-ray sources in the XMM-Newton serendipitous source catalog. LIN D., WEBB N.A. and BARRET D.
2013ApJS..206...14G 78             C       1 25 78 Optical counterparts of the nearest ultraluminous X-ray sources. GLADSTONE J.C., COPPERWHEAT C., HEINKE C.O., et al.
2013ApJ...776..100B 154           X         4 62 11 The local environment of ultraluminous X-ray sources viewed by XMM-newton's optical monitor. BERGHEA C.T., DUDIK R.P., TINCHER J., et al.
2013MNRAS.435.1758S 519       D     X C       13 22 179 The ultraluminous state revisited: fractional variability and spectral shape as diagnostics of super-Eddington accretion. SUTTON A.D., ROBERTS T.P. and MIDDLETON M.J.
2014MNRAS.444.2415S 789       D     X C       20 17 11 Irradiated, colour-temperature-corrected accretion discs in ultraluminous X-ray sources. SUTTON A.D., DONE C. and ROBERTS T.P.
2014ApJ...797...79W 15       D               3 44 24 Spatially resolving a starburst galaxy at hard X-ray energies: NuSTAR, Chandra, and VLBA observations of NGC 253. WIK D.R., LEHMER B.D., HORNSCHEMEIER A.E., et al.
2015NewA...37....1Z 24 3 On the black hole masses in ultra-luminous X-ray sources. ZHOU X.-L.
2015A&A...579A..22D 16       D               1 17 17 Searching for coherent pulsations in ultraluminous X-ray sources. DOROSHENKO V., SANTANGELO A. and DUCCI L.
2017ApJ...836...48S 492       D     X         13 16 5 Crossing the Eddington limit: examining disk spectra at high accretion rates. SUTTON A.D., SWARTZ D.A., ROBERTS T.P., et al.
2017A&A...608A..47K 176       D     X         5 39 81 ULX spectra revisited: Accreting, highly magnetized neutron stars as the engines of ultraluminous X-ray sources. KOLIOPANOS F., VASILOPOULOS G., GODET O., et al.
2021MNRAS.504..974G 43           X         1 4 4 Super-Eddington accretion on to a stellar mass ultraluminous X-ray source NGC 4190 ULX1. GHOSH T. and RANA V.
2023MNRAS.524.4302K 104       D         F     3 44 ~ Long-term X-ray/UV variability in ULXs. KHAN N. and MIDDLETON M.J.
2025ApJ...995...26Z 47           X         1 5 ~ Radiation GRMHD Models of Accretion onto Stellar-mass Black Holes. I. Survey of Eddington Ratios. ZHANG L., STONE J.M., MULLEN P.D., et al.

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