SIMBAD references

2012MNRAS.423.2425P - Mon. Not. R. Astron. Soc., 423, 2425-2435 (2012/July-1)

The young stellar cluster [DBS2003] 157 associated with the H II region GAL 331.31-00.34.

PINHEIRO M.C., ABRAHAM Z., COPETTI M.V.F., ORTIZ R., FALCETA-GONCALVES D.A. and ROMAN-LOPES A.

Abstract (from CDS):

We report a study of the stellar content of the near-infrared (NIR) cluster [DBS2003] 157 embedded in the extended H II region GAL 331.31-00.34, which is associated with the IRAS source 16085-5138. JHK photometry was carried out in order to identify potential ionizing candidates, and the follow-up NIR spectroscopy allowed the spectral classification of some sources, including two O-type stars. A combination of NIR photometry and spectroscopy data was used to obtain the distance of these two stars, with the method of spectroscopic parallax: IRS 298 (O6 V, 3.35±0.61 kpc) and IRS 339 (O9 V, 3.24±0.56 kpc). Adopting the average distance of 3.29±0.58 kpc and comparing the Lyman continuum luminosity of these stars with that required to account for the radio continuum flux of the H II region, we conclude that these two stars are the ionizing sources of GAL 331.31-00.34. Young stellar objects (YSOs) were searched by using our NIR photometry and mid-infrared (MIR) data from the Galactic Legacy Infrared Mid-Plane Survey Extraordinaire (GLIMPSE) survey. The analysis of NIR and MIR colour–colour diagrams resulted in 47 YSO candidates.

The GLIMPSE counterpart of IRAS 16085-5138, which presents IRAS colour indices compatible with an ultracompact H II region, has been identified. The analysis of its spectral energy distribution between 2 and {img}m revealed that this source shows a spectral index α= 3.6 between 2 and {img}m, which is typical of a YSO immersed in a protostellar envelope. Lower limits to the bolometric luminosity and the mass of the embedded protostar have been estimated as L= 7.7 {x} 103 L and M= 10 M, respectively, which correspond to a B0–B1 V zero-age main sequence star.

Based on observations carried at the Southern Observatory for Astrophysical Research (SOAR) observatory, a joint project of the Ministério de Ciência, Tecnologia e Inovação (MCTI) of the República Federativa do Brasil, the U.S. National Optical Astronomy Observatory (NOAO), the University of North Carolina at Chapel Hill (UNC) and the Michigan State University (MSU).


Abstract Copyright: 2012 The Authors Monthly Notices of the Royal Astronomical Society2012 RAS

Journal keyword(s): stars: early-type - stars: pre-main-sequence - H {sc ii} regions - Herbig–Haro objects

Nomenclature: Table A1: [PAC2012] IRS NNN N=91 among (Nos 3-533). Table 4: [PAC2012] CE NN (Nos 1-11).

Simbad objects: 105

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