Details on Acronym: [BBM2015] | |
[BBM2015] | (Britavskiy+Bonanos+Mehner+, 2015) |
Write: | <<[BBM2015] Phoenix NN>> <<[BBM2015] Pegasus NN>> <<[BBM2015] Sextans A NN>> <<[BBM2015] WLM NN>> |
N: | 14+19+15+31 |
Object: | (Mid IR) (SIMBAD class: Infrared = Infra-Red Source) |
Note: | VLT FORS2 multi-object spectroscopy of N=14+19+15+31 point sources in four star-forming dwarf irregular galaxies: Pegasus, Phoenix,Sextans A and WLM. Use of Spitzer IRAC data. See also [BBM2014] and [BBH2019]. |
in source: | NAME WLM Galaxy |
in source: | NAME Sextans A |
in source: | NAME Pegasus Dwarf Galaxy |
in source: | NAME Phe Galaxy |
Ref: | =2015A&A...584A..33B |
by | BRITAVSKIY N.E. , BONANOS A.Z., MEHNER A., BOYER M.L., McQUINN K.B.W. |
Astron. Astrophys., 584A, 33-33 (2015) | |
Identification of dusty massive stars in star-forming dwarf irregular galaxies in the Local Group with mid-IR photometry. | |
o | Table A.1: <[BBM2015] Phoenix NN> (Nos 1-14). Table A.2: <[BBM2015] Pegasus NN> (Nos 1-19). Table A.3: <[BBM2015] Sextans A NN> (Nos 1-15). Table A.4: <[BBM2015] WLM NN> (Nos 1-31). |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |