|
other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
| CXOU J133705.1-295207 , the SIMBAD biblio (20 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST09:12:36 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2012ApJ...750..152S | 291 | T A | S X C | 5 | 15 | 40 | The birth of an ultraluminous X-ray source in M83. | SORIA R., KUNTZ K.D., WINKLER P.F., et al. | |
| 2013MNRAS.428.2480E | 38 | X | 1 | 12 | 6 | Swift observations of the ultraluminous X-ray source XMMU J004243.6+412519 in M31. | ESPOSITO P., MOTTA S.E., PINTORE F., et al. | ||
|
2014ApJS..212...21L |
15 | D | 1 | 493 | 33 | A deep Chandra ACIS survey of M83. | LONG K.S., KUNTZ K.D., BLAIR W.P., et al. | ||
| 2015ApJ...799..140S | 2597 | A | S X | 66 | 12 | 7 | The slim-disk state of the ultraluminous X-ray source in M83. | SORIA R., KUNTZ K.D., LONG K.S., et al. | |
| 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. | ||
| 2015A&A...580A..71L | 39 | X | 1 | 10 | 4 | Swift-XRT six-year monitoring of the ultraluminous X-ray source M33 X-8. | LA PAROLA V., D'AI A., CUSUMANO G., et al. | ||
| 2016ApJ...824..107Y | 212 | D | S X C | 4 | 34 | 12 | A hard X-ray study of the normal star-forming galaxy M83 with nustar. | YUKITA M., HORNSCHEMEIER A.E., LEHMER B.D., et al. | |
| 2016ApJ...829...28B | 39 | X | 1 | 9 | 14 | A broadband X-ray spectral study of the intermediate-mass black hole candidate M82 X-1 with NuSTAR, Chandra, and Swift. | BRIGHTMAN M., HARRISON F.A., BARRET D., et al. | ||
| 2017MNRAS.469..886S | 40 | X | 1 | 15 | 16 | Outbursts of the intermediate-mass black hole HLX-1: a wind-instability scenario. | SORIA R., MUSAEVA A., WU K., et al. | ||
| 2017A&A...608A..47K | 136 | D | X | 4 | 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. | |
| 2018MNRAS.477L..90P | 40 | X | 1 | 13 | 10 | A new ultraluminous X-ray source in the galaxy NGC 5907. | PINTORE F., BELFIORE A., NOVARA G., et al. | ||
|
2020MNRAS.495..479R |
16 | D | 1 | 917 | ~ | A new radio catalogue for M83: supernova remnants and H II regions. | RUSSELL T.D., WHITE R.L., LONG K.S., et al. | ||
|
2021ApJ...912...31H |
17 | D | 1 | 337 | ~ | Calibrating X-ray binary luminosity functions via optical reconnaissance. I. The case of M83. | HUNT Q., GALLO E., CHANDAR R., et al. | ||
|
2021A&A...649A.104G |
602 | D | S X C | 13 | 26 | 23 | Long-term X-ray spectral evolution of ultraluminous X-ray sources: implications on the accretion flow geometry and the nature of the accretor. | GURPIDE A., GODET O., KOLIOPANOS F., et al. | |
| 2023A&A...669A.130A | 44 | X | 1 | 18 | ~ | The ultraluminous X-ray source M 81 X-6: a weakly magnetised neutron star with a precessing accretion disc? | AMATO R., GURPIDE A., WEBB N.A., et al. | ||
| 2023MNRAS.520.5724B | 47 | X | 1 | 5 | 19 | Understanding the high-mass binary black hole population from stable mass transfer and super-Eddington accretion in BPASS. | BRIEL M.M., STEVANCE H.F. and ELDRIDGE J.J. | ||
| 2023MNRAS.522.1377S | 87 | X | 2 | 49 | ~ | The largest bright ULX population in a galaxy: X-ray variability and luminosity function in the Cartwheel ring galaxy. | SALVAGGIO C., WOLTER A., BELFIORE A., et al. | ||
| 2023MNRAS.524.4302K | 104 | D | F | 3 | 44 | ~ | Long-term X-ray/UV variability in ULXs. | KHAN N. and MIDDLETON M.J. | |
| 2024MNRAS.52710185A | 179 | X | 4 | 20 | ~ | NGC 5474 X-1: A neutron star ultraluminous X-ray source in an old stellar cluster? | ATAPIN K., VINOKUROV A., SARKISYAN A., et al. | ||
| 2024ApJ...968...95M | 45 | X | 1 | 7 | ~ | Phase-dependent Spectral Shape Changes in the Ultraluminous X-Ray Pulsar NGC 5907 ULX1. | MIURA D., KOBAYASHI S.B. and YAMAGUCHI H. |