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IGR J05414-6858 , the SIMBAD biblio (15 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.24CEST23:10:51 |
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 |
---|---|---|---|---|---|---|---|---|---|
2012A&A...542A.109S | 1223 | T A | X C F | 29 | 9 | 12 |
Discovery of the neutron star spin and a possible orbital period from the Be/X-ray binary IGR J05414-6858 in the LMC. |
STURM R., HABERL F., RAU A., et al. | |
2010ATel.2695....1G | 76 | T | 1 | 5 | 4 |
New X-ray source IGR J05414-6858 discovered with INTEGRAL. |
GREBENEV S.A. and LUTOVINOV A.A. | ||
2010ATel.2696....1L | 76 | T | 1 | 2 | 2 |
Swift follow-up observations of a new transient source IGRJ05414-6858. |
LUTOVINOV A. and GREBENEV S. | ||
2010ATel.2704....1R | 153 | T | X | 3 | 5 | 3 |
IGR J05414-6858 is a Be-X-ray binary. |
RAU A., SCHADY P., GREINER J., et al. | |
2013MNRAS.428...50G | 234 | A | D | X C | 6 | 44 | 13 | Deep hard X-ray survey of the Large Magellanic Cloud. | GREBENEV S.A., LUTOVINOV A.A., TSYGANKOV S.S., et al. |
2013MNRAS.428.3607K | 39 | X | 1 | 12 | 8 | Swift J045106.8-694803: a highly magnetized neutron star in the Large Magellanic Cloud. | KLUS H., BARTLETT E.S., BIRD A.J., et al. | ||
2013A&A...551A..96S | 39 | X | 1 | 9 | 3 | RX J0123.4-7321, a Be/X-ray binary in the wing of the Small Magellanic Cloud. | STURM R., HABERL F., PIETSCH W., et al. | ||
2011ATel.3537....1S | 154 | T | X | 3 | 2 | 1 |
IGR J05414-6858 detected in X-ray outburst with SWIFT. |
STURM R., HABERL F., PIETSCH W., et al. | |
2016ApJS..223...15B | 16 | D | 1 | 945 | 98 | The IBIS soft gamma-ray sky after 1000 INTEGRAL orbits. | BIRD A.J., BAZZANO A., MALIZIA A., et al. | ||
2016MNRAS.459..140M | 96 | D | F | 2 | 172 | 4 | INTEGRAL/IBIS deep extragalactic survey: M81, LMC and 3C 273/Coma fields. | MEREMINSKIY I.A., KRIVONOS R.A., LUTOVINOV A.A., et al. | |
2016MNRAS.459..528A | 16 | D | 6 | 126 | 68 | Star formation history and X-ray binary populations: the case of the Large Magellanic Cloud. | ANTONIOU V. and ZEZAS A. | ||
2016ApJ...829...30C | 257 | D | X | 7 | 38 | 17 | Tracing the lowest propeller line in Magellanic high-mass X-ray binaries. | CHRISTODOULOU D.M., LAYCOCK S.G.T., YANG J., et al. | |
2018MNRAS.474.3228P | 41 | X | 1 | 33 | 6 | The 155-day X-ray cycle of the very massive Wolf-Rayet star Melnick 34 in the Large Magellanic Cloud. | POLLOCK A.M.T., CROWTHER P.A., TEHRANI K., et al. | ||
2022A&A...661A..25H | 18 | D | 1 | 52 | 10 | eROSITA calibration and performance verification phase: High-mass X-ray binaries in the Magellanic Clouds. | HABERL F., MAITRA C., CARPANO S., et al. | ||
2022ApJ...941..126H | 18 | D | 1 | 106 | ~ | Monte Carlo Simulations on Possible Collimation Effects of Outflows to Fan Beam Emission of Ultraluminous Accreting X-Ray Pulsars. | HOU X., YOU Y., JI L., et al. |