[HS80] B416 , the SIMBAD biblio

[HS80] B416 , the SIMBAD biblio (24 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST10:03:18


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Title First 3 Authors
1995AJ....110.2739C viz 38 18 An atlas of H-alpha emitting regions in M33: a systematic search for SS433 star candidates. CALZETTI D., KINNEY A.L., FORD H., et al.
1996AJ....112.1450C 59 22 LBV-type stars in M33. CORRAL L.J.
1996ApJ...469..629M viz 363 89 The UV-brightest stars of M33 and its nucleus: discovery, photometry, and optical spectroscopy. MASSEY P., BIANCHI L., HUTCHINGS J.B., et al.
1998IBVS.4595....1S 71 T       O           2 3 Periodic light variation in

B416,
a luminous blue star in M33.
SHEMMER O. and LEIBOWITZ E.M.
2000MNRAS.311..698S 108 T K                 4 11 Periodic microvariation of

B416,
a new luminous blue variable in M33.
SHEMMER O., LEIBOWITZ E.M. and SZKODY P.
2001PASP..113.1025T 274 7 Astrophysics in 2000. (Invited review). TRIMBLE V. and ASCHWANDEN M.J.
2003IAUS..212...38H 35 4 Luminous Blue Variables, cool hypergiants and some impostors in the H-R diagram. HUMPHREYS R.M.
2003RMxAC..16..265C 11 2 Luminous blue variables in the Local Universe. CORRAL L.J. and HERRERO A.
2004BaltA..13..156S 37   K                 2 4 B 416 - A b[e]-supergiant in interacting binary? SHOLUKHOVA O., FABRIKA S., ROTH M., et al.
2005A&A...437..217F 37   K                 7 20 Crowded field 3D spectroscopy of LBV candidates in M33. FABRIKA S., SHOLUKHOVA O., BECKER T., et al.
2006AJ....131.2478M viz 15       D               1 554 395 A survey of Local Group galaxies currently forming stars. I. UBVRI photometry of stars in M 31 and M 33. MASSEY P., OLSEN K.A.G., HODGE P.W., et al.
2006MNRAS.370.1429S viz 307 11 Long-term V-band monitoring of the bright stars of M33 at the Wise Observatory. SHPORER A. and MAZEH T.
2007AJ....134.2474M viz 89       D       C       2 392 140 A survey of local group galaxies currently forming stars. III. A search for luminous blue variables and other Hα emission-line stars. MASSEY P., McNEILL R.T., OLSEN K.A.G., et al.
2009ApJ...705.1364T viz 91       D         F     1 92 201 A new class of luminous transients and a first census of their massive stellar progenitors. THOMPSON T.A., PRIETO J.L., STANEK K.Z., et al.
2011AJ....141...18P 38           X         1 16 10 Optical spectrophotometric monitoring of the extreme luminous blue variable star GR 290 (Romano's star) in M 33. POLCARO V.F., ROSSI C., VIOTTI R.F., et al.
2012A&A...541A.146C 397       D     X C       10 74 32 On the nature of candidate luminous blue variables in M 33. CLARK J.S., CASTRO N., GARCIA M., et al.
2014ApJ...790...48H viz 1548     A D     X C       40 102 54 Luminous and variable stars in M31 and M33. II. Luminous blue variables, candidate LBVs, Fe II emission line stars, and other supergiants. HUMPHREYS R.M., WEIS K., DAVIDSON K., et al.
2015ApJ...800..118B 39           X         1 24 8 A newly recognized very young supernova remnant in M83. BLAIR W.P., WINKLER P.F., LONG K.S., et al.
2015A&A...581A..12B 195           X         5 13 4 Var C: Long-term photometric and spectral variability of a luminous blue variable in M33. BURGGRAF B., WEIS K., BOMANS D.J., et al.
2016AJ....152...62M viz 16       D               3 76 47 A spectroscopic survey of massive stars in M31 and M33. MASSEY P., NEUGENT K.F. and SMART B.M.
2017ApJ...836...64H viz 373       D     X         10 209 45 Luminous and variable stars in M31 and M33. IV. Luminous blue variables, candidate LBVs, B[e] supergiants, and the warm hypergiants: how to tell them apart. HUMPHREYS R.M., GORDON M.S., MARTIN J.C., et al.
2017ApJ...844...40H viz 254       D     X C       6 68 11 Luminous and variable stars in M31 and M33. V. The upper HR diagram. HUMPHREYS R.M., DAVIDSON K., HAHN D., et al.
2018MNRAS.480.3706K 658       D     X C       16 20 6 On the evolutionary state of massive stars in transition phases in M33. KOURNIOTIS M., KRAUS M., ARIAS M.L., et al.
2018AJ....156..294A 16       D               2 106 7 Shedding light on the isolation of luminous blue variables. AADLAND E., MASSEY P., NEUGENT K.F., et al.

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