2018A&A...612A..36D


C.D.S. - SIMBAD4 rel 1.7 - 2019.11.12CET08:08:43

2018A&A...612A..36D - Astronomy and Astrophysics, volume 612A, 36-36 (2018/4-1)

Radio and infrared study of southern H II regions G346.056-0.021 and G346.077-0.056.

DAS S.R., TEJ A., VIG S., LIU T., GHOSH S.K. and CHANDRA C.H.I.

Abstract (from CDS):

Aim. We present a multiwavelength study of two southern Galactic H II regions G346.056-0.021 and G346.077-0.056 which are located at a distance of 10.9 kpc. The distribution of ionized gas, cold and warm dust, and the stellar population associated with the two H II regions are studied in detail using measurements at near-infrared, mid-infrared, far-infrared, submillimeter and radio wavelengths.
Methods. The radio continuum maps at 1280 and 610MHz were obtained using the Giant Metrewave Radio Telescope to probe the ionized gas. The dust temperature, column density, and dust emissivity maps were generated using modified blackbody fits in the far-infrared wavelength range 160-500 µm. Various near- and mid-infrared color and magnitude criteria were adopted to identify candidate ionizing star(s) and the population of young stellar objects in the associated field.
Results. The radio maps reveal the presence of diffuse ionized emission displaying distinct cometary morphologies. The 1280MHz flux densities translate to zero age main sequence spectral types in the range O7.5V-O7V and O8.5V-O8V for the ionizing stars of G346.056-0.021 and G346.077-0.056, respectively. A few promising candidate ionizing star(s) are identified using near-infrared photometric data. The column density map shows the presence of a large, dense dust clump enveloping G346.077-0.056. The dust temperature map shows peaks towards the two H II regions. The submillimeter image shows the presence of two additional clumps, one being associated with G346.056-0.021. The masses of the clumps are estimated to range between ∼1400 and 15250M. Based on simple analytic calculations and the correlation seen between the ionized gas distribution and the local density structure, the observed cometary morphology in the radio maps is better explained invoking the champagne-flow model.

Abstract Copyright: © ESO 2018

Journal keyword(s): infrared: ISM - radio continuum: ISM - HII regions - ISM: individual objects: G346.056-0.021 - ISM: individual objects: G346.077-0.056

VizieR on-line data: <Available at CDS (J/A+A/612/A36): list.dat fits/*>

Simbad objects: 19

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Number of rows : 19

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2020
#notes
1 3C 48 QSO 01 37 41.2995845985 +33 09 35.079126038   16.62 16.20     ~ 2431 2
2 3C 286 Sy1 13 31 08.2885060664 +30 30 32.960825108   17.51 17.25     ~ 3617 1
3 [CPA2006] S51 bub 16 19 48 -51 02.6           ~ 8 0
4 NVSS J162914-300003 Rad 16 29 14.9 -30 00 01           ~ 6 1
5 2MASS J17073981-4031414 * 17 07 39.81144 -40 31 41.4300           ~ 1 0
6 2MASS J17074015-4031519 * 17 07 40.15824 -40 31 51.9384           ~ 1 0
7 2MASS J17074045-4031118 * 17 07 40.4538942604 -40 31 11.831730645           ~ 1 0
8 HRDS G346.056-00.021 HII 17 07 40.5 -40 31 38           ~ 5 0
9 2MASS J17074099-4031400 * 17 07 40.99440 -40 31 40.0296           ~ 1 0
10 2MASS J17074166-4031240 * 17 07 41.66328 -40 31 24.0456           ~ 1 0
11 2MASS J17074302-4031339 * 17 07 43.02192 -40 31 33.9348           ~ 1 0
12 2MASS J17075294-4031343 * 17 07 52.9288927962 -40 31 34.521322560           ~ 1 0
13 2MASS J17075324-4031308 * 17 07 53.2443659888 -40 31 30.831793498           ~ 1 0
14 2MASS J17075398-4031348 * 17 07 53.98224 -40 31 34.8528           ~ 1 0
15 VVV CL094 Cl* 17 07 54 -40 31.6           ~ 3 0
16 HRDS G346.077-00.056 HII 17 07 54.1 -40 31 36           ~ 4 0
17 MSX6C G346.0774-00.0562 HII 17 07 54.216 -40 31 35.40           ~ 8 0
18 2MASS J17075484-4031451 * 17 07 54.84864 -40 31 45.1668           ~ 1 0
19 2MASS J17075523-4031408 * 17 07 55.2351705295 -40 31 40.869109797           ~ 1 0

    Equat.    Gal    SGal    Ecl

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2019.11.12-08:08:43

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