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| OGLE J050722.23-684759.1 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST20:45:23 |
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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 |
|---|---|---|---|---|---|---|---|---|---|
2002AJ....124.2039K 
|
1271 | 32 | Blue variable stars from the MACHO database. I. Photometry and spectroscopy of the Large Magellanic Cloud sample. | KELLER S.C., BESSELL M.S., COOK K.H., et al. | |||||
|
2005MNRAS.361.1055S
|
15 | D | 1 | 2408 | 24 | Be star candidates in the Large Magellanic Cloud: the catalogue and comparison with the Small Magellanic Cloud sample. | SABOGAL B.E., MENNICKENT R.E., PIETRZYNSKI G., et al. | ||
| 2018MNRAS.475.3253V | 96 | D | F | 6 | 26 | 3 | Identification of high-mass X-ray binaries selected from XMM-Newton observations of the LMC. | VAN JAARSVELD N., BUCKLEY D.A.H., McBRIDE V.A., et al. | |
| 2021MNRAS.504..326M | 1839 | T K A | D | S X C F | 41 | 19 | 13 |
XMMU J050722.1-684758: discovery of a new Be X-ray binary pulsar likely associated with the supernova remnant MCSNR J0507-6847. |
MAITRA C., HABERL F., MAGGI P., et al. |
|
2021MNRAS.505.5567V
|
17 | D | 1 | 3400 | ~ | Red Be stars in the Magellanic Clouds? | VIEIRA K., GARCIA-VARELA A., SABOGAL B., et al. | ||
| 2021ApJ...920...67X | 268 | D | X C | 6 | 14 | ~ | Population synthesis of neutron star X-ray binaries associated with supernova remnants. | XING Z.-P. and LI X.-D. | |
| 2022MNRAS.511.4447K | 17 | D | 1 | 8 | 1 | Origin of young accreting neutron stars in high-mass X-ray binaries in supernova remnants. | KHOKHRIAKOVA A.D. and POPOV S.B. | ||
| 2023MNRAS.523.5510G | 44 | X | 1 | 15 | ~ | SALT spectroscopy of the HMXB associated with the LMC supernova remnant MCSNR J0513-6724. | GVARAMADZE V.V., KNIAZEV A.Y., CASTRO N., et al. | ||
|
2024A&A...692A.237Z
|
45 | X | 1 | 127 | ~ | First study of the supernova remnant population in the Large Magellanic Cloud with eROSITA. | ZANGRANDI F., JURK K., SASAKI M., et al. |
