[BE74] 544 , the SIMBAD biblio

[BE74] 544 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST17:37:04


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Title First 3 Authors
1974A&AS...18...47B 627 74 H alpha emission-line stars in the Large Magellanic Cloud. I. A new deep survey. BOHANNAN B. and EPPS H.W.
2000AJ....119.2214M viz 653 146 The progenitor masses of Wolf-Rayet stars and luminous blue variables determined from cluster turnoffs. I. Results from 19 OB associations in the Magellanic clouds. MASSEY P., WATERHOUSE E. and DEGIOIA-EASTWOOD K.
2002AJ....124.2039K viz 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 viz 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.
2009AJ....138.1003B viz 15       D               1 1760 163 Spitzer SAGE infrared photometry of massive stars in the Large Magellanic Cloud. BONANOS A.Z., MASSA D.L., SEWILO M., et al.
2012MNRAS.425..355R viz 15       D               1 589 26 Emission-line stars discovered in the UKST hα survey of the large Magellanic cloud – I. Hot stars. REID W.A. and PARKER Q.A.
2012A&A...548A..16H viz 15       D               1 627 3 Improved astrometry for the Bohannan & Epps catalogue. HOWARTH I.D.
2013A&A...555A.141H viz 15       D               1 1714 3 Emission-line stars in the LMC: the Armagh survey and a metacatalogue. HOWARTH I.D.
2013AcA....63..159U viz 15       D               1 768 16 Variable stars from the OGLE-III Shallow Survey in the Large Magellanic Cloud. ULACZYK K., SZYMANSKI M.K., UDALSKI A., et al.
2021MNRAS.505.5567V viz 17       D               1 3400 ~ Red Be stars in the Magellanic Clouds? VIEIRA K., GARCIA-VARELA A., SABOGAL B., et al.
2023ApJ...952...64L viz 17       D               1 2632 ~ Massive Hypervelocity Runaway Stars in the Large Magellanic Cloud. LIN Z., XU Y., HAO C., et al.

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