Dictionary of Nomenclature of Celestial Objects
(Last update: 22-Mar-2024)

Result of query: info cati MNM2015] SMCeNNN-N$
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Details on Acronym:   [MNM2015]
  
[MNM2015] (Massey+Neugent+Morrell, 2015)
Write:<<[MNM2015] {LMCe|SMCe}NNN-N>>
<<[MNM2015] LMCNNN-N>>
N: 22+4+3
Object:WR + Em* + *  (SIMBAD class: Star)
Note:Las Campanas 1m Swope telescope imaging and Magellan 6.5 Clay telescope MagE spectroscopy of N=4 WR stars, N=2 emission-line stars, N=6 B-type stars and N=1 RR Lyr variable.
The letter "e" in format denotes the e2v fields to distinguish them from the numbering system used in Paper I (Massey et al. 2014ApJ...788...83M).
See also [MNM2014].
Ref:=2015ApJ...807...81M
byMASSEY P. , NEUGENT K.F., MORRELL N.
 Astrophys. J., 807, 81 (2015)
  A modern search for Wolf-Rayet stars in the Magellanic Clouds. II. A second year of discoveries.
oTables 1-3: <[MNM2015] LMCeNNN-N> N=8, <[MNM2015] SMCeNNN-N> N=2, <[MNM2015] LMCNNN-N> N=3.
Ref:=2017ApJ...837..122M
byMASSEY P. , NEUGENT K.F., MORRELL N.
 Astrophys. J., 837, 122-122 (2017)
  A modern search for Wolf-Rayet stars in the Magellanic Clouds. III. A third year of discoveries.
oTables 1-3: <[MNM2015] LMCeNNN-N> N=14 added, <[MNM2015] SMCeNNN-N> N=2 added.
Originof the Acronym: S = Created by Simbad, the CDS Database