1997A&A...325..282C


Query : 1997A&A...325..282C

1997A&A...325..282C - Astronomy and Astrophysics, volume 325, 282-294 (1997/9-1)

The molecular environment of H2O masers: VLA ammonia observations.

CODELLA C., TESTI L. and CESARONI R.

Abstract (from CDS):

We present the results of single dish and interferometric observations of ammonia towards 5 sources selected from a sample of H2O and OH masers associated with star forming regions. The Medicina telescope was used to observe the NH3(1,1), (2,2), and (3,3) inversion transitions. High resolution maps in the NH3(2,2) and (3,3) lines and in the 1.3 cm continuum were then obtained with the Very Large Array. The main result of this research is to confirm the belief that H2O masers form in hot dense molecular cores which are sites of massive star formation. We also find evidence for the H2O maser phase to be prior to the appearance of an ultracompact HII region around the embedded high mass star(s).

Abstract Copyright:

Journal keyword(s): masers - stars: formation - interstellar medium: molecules - radio lines: interstellar

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 - 2022
#notes
1 NAME W 3 OH HII 02 27 04.1 +61 52 22           ~ 981 2
2 W 3(H2O) Mas 02 27 04.6 +61 52 25           ~ 135 0
3 MMB G012.681-00.182 cor 18 13 54.7457 -18 01 46.588           ~ 51 0
4 IRAS 18182-1433 mul 18 21 07.9 -14 31 53           ~ 100 0
5 OH 16.59 -0.05 cor 18 21 09.2137 -14 31 45.484           ~ 119 0
6 Caswell OH 023.01-00.41 Mas 18 34 40.5 -09 00 39           ~ 11 0
7 GAL 024.78+00.08 HII 18 36.2 -07 13           ~ 79 0
8 Caswell OH 024.78+00.08 Mas 18 36 12.5 -07 12 10           ~ 18 0
9 GAL 028.86-00.07 HII 18 43 45.8 -03 35 30           ~ 26 0
10 Caswell OH 028.86+00.07 Mas 18 43 48.1 -03 35 31           ~ 15 0
11 GRS G081.70 +00.50 SFR 20 39 01.6 +42 19 38           O4.5 1001 0

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2022.05.20-18:26:53

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