2023MNRAS.524.4384P


Query : 2023MNRAS.524.4384P

2023MNRAS.524.4384P - Mon. Not. R. Astron. Soc., 524, 4384-4402 (2023/September-3)

SCOTCH - search for clandestine optically thick compact H IIs.

PATEL A.L., URQUHART J.S., YANG A.Y., MOORE T.J.T., MENTEN K.M., THOMPSON M.A., HOARE M.G., IRABOR T., BREEN S.L. and SMITH M.D.

Abstract (from CDS):

This study uses archival high-frequency continuum data to expand the search for Hypercompact H II regions and determine the conditions at which they appear, as this stage high mass star formation is short-lived and rare. We use 23 GHz continuum data taken towards methanol masers, which are an excellent signpost for very young embedded high-mass protostars. We have searched for high-frequency, optically thick radio sources to identify HC H II region candidates. The data cover 128 fields that include 141 methanol masers identified by the Methanol Multibeam (MMB) survey. We have detected 68 high-frequency radio sources and conducted a multiwavelength analysis to determine their nature. This has identified 49 H II regions, 47 of which are embedded in dense clumps fourteen of which do not have a 5 GHz radio counterpart. We have identified 13 methanol maser sites that are coincident with radio sources that have a steep positive spectral index. The majority of these are not detected in the mid-infrared and have been classified as protostellar or young stellar objects in the literature and we therefore consider to be good HC H II region candidates, however, further work and higher resolution data are needed to confirm these candidates.

Abstract Copyright: © 2023 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society.

Journal keyword(s): stars: evolution - stars: formation - H ii regions - radio continuum: stars

Status at CDS : All or part of tables of objects could be ingested in SIMBAD with priority 2.

Simbad objects: 28

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Number of rows : 28
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 Caswell CH3OH 326.475+00.703 Mas 15 43 16.64 -54 07 14.6           ~ 10 0
2 [GMB2007b] J154316.9-540715 smm 15 43 16.9 -54 07 15           ~ 18 1
3 IRAS 15394-5358 Y*O 15 43 18.97320 -54 07 35.6448           ~ 40 0
4 MMB G331.710+00.603 cor 16 10 01.77 -50 49 32.3           ~ 23 0
5 AGAL G331.546-00.067 cor 16 12 10 -51 25.7           ~ 21 0
6 IRAS 16084-5127 Y*O 16 12 12.45528 -51 35 09.9888           ~ 33 0
7 OH 332.826-00.549 Mas 16 20 10.85 -50 53 14.2           ~ 16 0
8 AGAL G332.826-00.549 cor 16 20 11 -50 53.2           ~ 28 0
9 IRAS 16167-5036 Y*O 16 20 37.81920 -50 43 49.7136           ~ 27 0
10 Caswell CH3OH 336.983-00.183 Mas 16 36 12.41 -47 37 58.2           ~ 25 0
11 IRAS 16325-4731 cor 16 36 12.41856 -47 37 57.8280           ~ 29 0
12 OH 338.28+00.54 Y*O 16 38 09.109 -46 11 04.00           ~ 34 0
13 OH 338.925+00.557 Mas 16 40 33.53 -45 41 37.1           ~ 13 0
14 AGAL G338.926+00.554 cor 16 40 34 -45 41.7           ~ 37 0
15 MMB G338.566+00.110 Mas 16 41 07.03 -46 15 28.3           ~ 6 0
16 AGAL G338.567+00.109 smm 16 41 07.078 -46 15 29.34           ~ 13 0
17 OH 339.6-00.1 Y*O 16 46 05.99 -45 36 43.3           ~ 86 0
18 MMB G339.681-01.208 Mas 16 51 06.21 -46 16 02.9           ~ 4 0
19 MMB G339.682-01.207 Mas 16 51 06.23 -46 15 58.1           ~ 4 0
20 AGAL G339.681-01.209 smm 16 51 07 -46 16.1           ~ 12 0
21 MMB G004.676+00.276 Mas 17 55 18.34 -24 46 45.3           ~ 12 0
22 OH 005.90-00.38 Mas 18 00 30.373 -24 04 00.96           ~ 51 1
23 AGAL G005.884-00.392 smm 18 00 30.408 -24 03 59.66           ~ 25 0
24 MMB G012.112-00.126 Mas 18 12 33.39 -18 30 07.6           ~ 15 0
25 MMB G014.230-00.509 cor 18 18 12.59 -16 49 22.8           ~ 25 0
26 [CUS2014] G018.7344-0.2261 cor 18 25 56 -12 42.8           ~ 34 0
27 MMB G018.735-00.227 Mas 18 25 56.46 -12 42 50.0           ~ 3 0
28 ICRF J193925.0-634245 Sy2 19 39 25.0245304992 -63 42 45.640373400   18.87 18.37 17.64   ~ 1332 2

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