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., Smith, M. D. and others. (2023) SCOTCH − search for clandestine optically thick compact H IIs. Monthly Notices of the Royal Astronomical Society, 524 (3). pp. 4384-4402. ISSN 1365-2966. E-ISSN 1365-2966. (doi:10.1093/mnras/stad2143) (KAR id:102231)
|
PDF
Publisher pdf
Language: English
This work is licensed under a Creative Commons Attribution 4.0 International License.
|
|
|
Download this file (PDF/4MB) |
Preview |
| Request a format suitable for use with assistive technology e.g. a screenreader | |
|
PDF
Author's Accepted Manuscript
Language: English |
|
|
Download this file (PDF/14MB) |
Preview |
| Request a format suitable for use with assistive technology e.g. a screenreader | |
| Official URL: https://doi.org/10.1093/mnras/stad2143 |
|
| Additional URLs: |
|
Abstract
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 multi-wavelength 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.
| Item Type: | Article |
|---|---|
| DOI/Identification number: | 10.1093/mnras/stad2143 |
| Uncontrolled keywords: | Space and Planetary Science; Astronomy and Astrophysics; stars evolution; stars formation; (ISM:) HII regions; radio continuum stars |
| Subjects: |
Q Science Q Science > QB Astronomy > QB460 Astrophysics |
| Institutional Unit: | Schools > School of Engineering, Mathematics and Physics > Physics and Astronomy |
| Former Institutional Unit: |
Divisions > Division of Natural Sciences > Physics and Astronomy
|
| Funders: | University of Kent (https://ror.org/00xkeyj56) |
| SWORD Depositor: | JISC Publications Router |
| Depositing User: | James Urquhart |
| Date Deposited: | 27 Jul 2023 13:51 UTC |
| Last Modified: | 22 Jul 2025 09:16 UTC |
| Resource URI: | https://kar.kent.ac.uk/id/eprint/102231 (The current URI for this page, for reference purposes) |
- Link to SensusAccess
- Export to:
- RefWorks
- EPrints3 XML
- BibTeX
- CSV
- Depositors only (login required):

https://orcid.org/0000-0001-5800-6710
Altmetric
Altmetric