Details on Acronym: [SDA2014] | |
[SDA2014] | (Sadavoy+Di Francesco+Andre+, 2014) |
Write: | <<[SDA2014] {West|East}NNN>> |
N: | 28 |
Object: | Poss. YSO (SIMBAD class: YSO_Candidate = Young Stellar Object Candidate) |
Note: | N=28 candidate Class 0 protostars in the Perseus molecular cloud. Use of PACS and SPIRE continuum data at 160µm, 250µm, 350µm, 500µm from the Herschel Gould Belt Survey. |
in source: | NAME Perseus Molecular Cloud |
Ref: | =2014ApJ...787L..18S |
by | SADAVOY S.I. , DI FRANCESCO J., ANDRE Ph., PEZZUTO S., BERNARD J.-P., MAURY A., MEN'SHCHIKOV A., MOTTE F., NGUYEN-LUONG Q., SCHNEIDER N., ARZOUMANIAN D., BENEDETTINI M., BONTEMPS S., ELIA D., HENNEMANN M., HILL T., KONYVES V., LOUVET F., PERETTO N., ROY A., WHITE G.J. |
Astrophys. J., 787L, 18 (2014) | |
Class 0 protostars in the Perseus molecular cloud: a correlation between the youngest protostars and the dense gas distribution. | |
o | Table 1: <[SDA2014] WestNNN> N=23 among (Nos West4-West162), <[SDA2014] EastNN> N=5 among (Nos East4-East17). |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |