SIMBAD references

2011MNRAS.418.1689U - Mon. Not. R. Astron. Soc., 418, 1689-1706 (2011/December-2)

The red MSX source survey: ammonia and water maser analysis of massive star-forming regions.

URQUHART J.S., MORGAN L.K., FIGURA C.C., MOORE T.J.T., LUMSDEN S.L., HOARE M.G., OUDMAIJER R.D., MOTTRAM J.C., DAVIES B. and DUNHAM M.K.

Abstract (from CDS):

The Red MSX Source (RMS) survey has identified a sample of ∼ 1200 massive young stellar objects (MYSOs), compact and ultra-compact H II regions from a sample of ∼ 2000 MSX and Two Micron All Sky Survey (2MASS) colour-selected sources. We have used the 100-m Green Bank Telescope to search for 22–24 GHz water maser and ammonia (1,1), (2,2) and (3,3) emission towards ∼ 600 RMS sources located within the northern Galactic plane. We have identified 308 H2 O masers which corresponds to an overall detection rate of ∼ 50 per cent. We find no significant difference in the detection rate for H II regions and MYSOs which would suggest that the conditions required to produce maser emission are equally likely in both phases. Comparing the detection rates as a function of luminosity, we find the H2 O detection rate has a positive dependence on the source luminosity, with the detection rate increasing with increasing luminosity.

We detect ammonia emission towards 479 of these massive young stars, which corresponds to ∼ 80 per cent. Ammonia is an excellent probe of high-density gas allowing us to measure key parameters such as gas temperatures, opacities and column densities, as well as providing an insight into the gas kinematics. The average kinetic temperature, full width at half-maximum linewidth and total NH3 column density for the sample are approximately 22 K, 2 km/s and 2 {x} 1015/cm2, respectively. We find that the NH3(1,1) linewidth and kinetic temperature are correlated with luminosity, and finding no underlying dependence of these parameters on the evolutionary phase of the embedded sources, we conclude that the observed trends in the derived parameters are more likely to be due to the energy output of the central source and/or the linewidth–clump mass relationship.

The velocities of the peak H2 O masers and the NH3emission are in excellent agreement with each other, which would strongly suggest an association between the dense gas and the maser emission. Moreover, we find the bolometric luminosity of the embedded source and the isotropic luminosity of the H2 O maser are also correlated. We conclude from the correlations of the cloud and water maser velocities and the bolometric and maser luminosity that there is a strong dynamical relationship between the embedded young massive star and the H2 O maser.


Abstract Copyright: 2011 CSIRO Monthly Notices of the Royal Astronomical Society2011 RAS

Journal keyword(s): stars: early-type - stars: formation - ISM: molecules - radio lines: ISM

VizieR on-line data: <Available at CDS (J/MNRAS/418/1689): table2.dat table5.dat h2o_data/* h2o_plots/* nh3_data/* nh3_plots/*>

Simbad objects: 596

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:2011MNRAS.418.1689U and select 'bookmark this link' or equivalent in the popup menu


2020.11.24-10:21:54

© Université de Strasbourg/CNRS

    • Contact