2002A&A...390L...1F

Query : 2002A&A...390L...1F

2002A&A...390L...1F - Astronomy and Astrophysics, volume 390L1-4 (2002/7-4)

G24.78+0.08: A cluster of high-mass (proto)stars.

FURUYA R.S., CESARONI R., CODELLA C., TESTI L., BACHILLER R. and TAFALLA M.

Abstract (from CDS):

We present the results of high angular resolution observations at millimeter wavelengths of the high-mass star forming region G24.78+0.08, where a cluster of four young stellar objects is detected. We discuss evidence for these to be high-mass (proto)stars in different evolutionary phases. One of the sources is detected only in the continuum at 2 and 2.6 mm and we suggest it may represent a good candidate of a high-mass protostar.

Abstract Copyright: ∼

Journal keyword(s): stars: formation - radio lines: ISM - ISM: jets and outflows - ISM: individual objects: G24.78+0.08

Nomenclature: Fig.1, Table 1: [FCC2002] A (Nos A-D).

Simbad objects: 11

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Number of rows : 11
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 NAME W 3 OH HII 02 27 04.1 +61 52 22           ~ 1064 2
2 W 3(H2O) Mas 02 27 04.6 +61 52 25           ~ 154 0
3 GAL 024.78+00.08 HII 18 36.2 -07 13           ~ 89 0
4 Caswell CH3OH 024.79+00.08 Mas 18 36 12.1 -07 12 13           ~ 8 0
5 NAME GAL 024.78+00.08 d Y*O 18 36 12.1 -07 11 59           ~ 5 0
6 Caswell OH 024.78+00.08 Mas 18 36 12.5 -07 12 10           ~ 18 0
7 [FCC2002] A Y*O 18 36 12.5 -07 12 08           ~ 5 0
8 [FC2000] G024.79+0.08 A HII 18 36 12.56 -07 12 10.8           ~ 3 0
9 [FCC2002] B Y*O 18 36 12.6 -07 12 09           ~ 8 0
10 [FC2000] G024.79+0.08 B HII 18 36 12.69 -07 12 14.5           ~ 2 0
11 NAME GAL 024.78+00.08 c Y*O 18 36 13.2 -07 11 59           ~ 10 0

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