SIMBAD references

2016A&A...595A..27G - Astronomy and Astrophysics, volume 595A, 27-27 (2016/11-1)

Toward gas exhaustion in the W51 high-mass protoclusters.

GINSBURG A., GOSS W.M., GODDI C., GALVAN-MADRID R., DALE J.E., BALLY J., BATTERSBY C.D., YOUNGBLOOD A., SANKRIT R., SMITH R., DARLING J., KRUIJSSEN J.M.D. and LIU H.B.

Abstract (from CDS):

We present new JVLA observations of the high-mass cluster-forming region W51A from 2 to 16 GHz with resolution θfwhm~=0.3-0.5''. The data reveal a wealth of observational results: (1) Currently forming, very massive (proto-O) stars are traced by o-H2CO21,1-21,2 emission, suggesting that this line can be used efficiently as a massive protostar tracer; (2) there is a spatially distributed population of ≲mJy continuum sources, including hypercompact HII regions and candidate colliding wind binaries, in and around the W51 proto-clusters; and (3) there are two clearly detected protoclusters, W51e and W51 IRS2, that are gas-rich but may have most of their mass in stars within their inner ≤0.05pc. The majority of the bolometric luminosity in W51 most likely comes from a third population of OB stars between these clusters. The presence of a substantial population of exposed O-stars coincident with a population of still-forming massive stars, together with a direct measurement of the low mass loss rate via ionized gas outflow from W51 IRS2, implies that feedback is ineffective at halting star formation in massive protoclusters. Instead, feedback may shut off the large-scale accretion of diffuse gas onto the W51 protoclusters, implying that they are evolving toward a state of gas exhaustion rather than gas expulsion. Recent theoretical models predict gas exhaustion to be a necessary step in the formation of gravitationally bound stellar clusters, and our results provide an observational validation of this process.

Abstract Copyright: © ESO, 2016

Journal keyword(s): HII regions - circumstellar matter - radio continuum: ISM - radio lines: ISM - stars: massive - stars: protostars

VizieR on-line data: <Available at CDS (J/A+A/595/A27): phot.dat list.dat fits/*>

Nomenclature: Fig. 2, Table 3: W51aNN (Nos W51d3-d7, W51e9-e23) added. Figs 2+A.2, Tables 3-8: [GGG2016] arc N=1, [GGG2016] W51aNNw (Nos W51d3, W51d4e-W51d4w, W51d5-W51d7, W51e8n-W51e8s, W51e9-23), [GGG2016] W51aNNd (Nos W51d3d, W51e11d, W51e18d), [GGG2016] W51aNNmol (Nos W51e8mol, W51e10mol).

Status in Simbad:  will not be processed

Simbad objects: 29

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2019.12.11-03:32:47

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