CH3OH and H2O masers in high-mass star-forming regions

By H. Beuther, A. Walsh, Peter Schilke, Sridharan T. K., K. Menten, F. Wyrowski. 2002

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We present a comparison of Class ii CH3OH (6.7 GHz) and H2O (22.2 GHz) masers at high spatial resolution in a sample of 29 massive star-forming regions. Absolute positions of both maser types are compared with mm dust continuum, cm continuum and mid-infrared sources. All maser features - regardless of the species - are associated with massive mm cores, but only 3 out of 18 CH3OH masers and 6 out of 22 H2O masers are associated with cm emission likely indicating the presence of a recently ignited massive star. These observations of a homogenous sample of massive, young star-forming regions confirm earlier results, obtained for each maser species separately, that both maser types are signposts of high-mass star formation in very early evolutionary stages. The data are consistent with models that explain CH3OH maser emission by radiative pumping in moderately hot cores, requiring the absence, or only weak, free-free cm continuum radiation due to recently ignited stars. Mid-infrared sources are associated with both maser types in approximately 60% of the observed fields. Thus, mid-infrared objects may power maser sites, but the detection of strong mid-infrared emission is not strictly necessary because it might be heavily extincted. A comparison of the spatial separations between the dierent observed quantities and other properties of the star-forming regions does not reveal any correlation. Our data suggest that CH3OH and H2O masers need a similar environment (dense and warm molecular gas), but that, due to the dierent excitation processes (radiative pumping for CH3OH and collisional pumping for H2O), no spatial correlations exist. Spatial associations are probably coincidences due to insucient angular resolution and projection eects. The kinematic structures we find in the dierent maser species show no recognizable pattern, and we cannot draw firm conclusions as to whether the features are produced in disks, outflows or expanding shock waves.

Subfields: Astronomy and Astrophysics, Atmospheric Science, Spectroscopy

View Paper: https://www.semanticscholar.org/paper/f4f8108cc0b5590fc11a60ff788ffc45420abbb6

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Citations in the corpus

ATLASGAL — towards a complete sample of massive star forming clumps ⋆ (2014, background): “For aspect ratios less than 2, the value a2 ∼ 1, which is suitable for this sample of clumps, and the value of a1 ∼ 1.3 (e.g. see Beuther et al. 2002 and Paper II for more details).”
The 6-GHz methanol multibeam maser catalogue – II. Galactic longitudes 6° to 20° (2010, background): “The other major targeted observations preceding the MMB survey were: Schutte et al. (1993); van der Walt et al. (1995); Caswell et al. (1995a); Walsh et al. (1997, 1998); Slysh et al. (1999); Szymczak et al. (2000); Beuther et al. (2002).”
ATLASGAL - The APEX telescope large area survey of the galaxy at 870 μm (2009, background): “…showing far-infrared (FIR) colors typical of ultra-compact Hii regions (Wood & Churchwell 1989), e.g., in high-density molecular tracers (Bronfman et al. 1996; Molinari et al. 1996), dust continuum emission (Faúndez et al. 2004), or maser emission (e.g., Palla et al. 1993; Beuther et al. 2002).”