An AST/RO Survey of CO(4-3) in ultracompact HII regions

The Antarctic Submillimeter Telescope and Remote Observatory (AST/RO) has been used to observe 78 of the IRAS point sources identified by Bronfman et al. (1996) as likely ultracompact HII regions. Results for the CO(4-3) line at 461.041GHz are presented. The 74 sources detected are bright and in man...

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Main Author: Walsh, Wilfred
Format: Report
Language:unknown
Published: arXiv 2003
Subjects:
Online Access:https://dx.doi.org/10.48550/arxiv.astro-ph/0306075
https://arxiv.org/abs/astro-ph/0306075
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spelling ftdatacite:10.48550/arxiv.astro-ph/0306075 2023-05-15T13:52:05+02:00 An AST/RO Survey of CO(4-3) in ultracompact HII regions Walsh, Wilfred 2003 https://dx.doi.org/10.48550/arxiv.astro-ph/0306075 https://arxiv.org/abs/astro-ph/0306075 unknown arXiv Assumed arXiv.org perpetual, non-exclusive license to distribute this article for submissions made before January 2004 http://arxiv.org/licenses/assumed-1991-2003/ Astrophysics astro-ph FOS Physical sciences Preprint Article article CreativeWork 2003 ftdatacite https://doi.org/10.48550/arxiv.astro-ph/0306075 2022-04-01T16:33:39Z The Antarctic Submillimeter Telescope and Remote Observatory (AST/RO) has been used to observe 78 of the IRAS point sources identified by Bronfman et al. (1996) as likely ultracompact HII regions. Results for the CO(4-3) line at 461.041GHz are presented. The 74 sources detected are bright and in many cases compact, making them potentially suitable as pointing calibrators for single dish submillimeter telescopes. : To be submitted to ApJS Report Antarc* Antarctic DataCite Metadata Store (German National Library of Science and Technology) Antarctic The Antarctic
institution Open Polar
collection DataCite Metadata Store (German National Library of Science and Technology)
op_collection_id ftdatacite
language unknown
topic Astrophysics astro-ph
FOS Physical sciences
spellingShingle Astrophysics astro-ph
FOS Physical sciences
Walsh, Wilfred
An AST/RO Survey of CO(4-3) in ultracompact HII regions
topic_facet Astrophysics astro-ph
FOS Physical sciences
description The Antarctic Submillimeter Telescope and Remote Observatory (AST/RO) has been used to observe 78 of the IRAS point sources identified by Bronfman et al. (1996) as likely ultracompact HII regions. Results for the CO(4-3) line at 461.041GHz are presented. The 74 sources detected are bright and in many cases compact, making them potentially suitable as pointing calibrators for single dish submillimeter telescopes. : To be submitted to ApJS
format Report
author Walsh, Wilfred
author_facet Walsh, Wilfred
author_sort Walsh, Wilfred
title An AST/RO Survey of CO(4-3) in ultracompact HII regions
title_short An AST/RO Survey of CO(4-3) in ultracompact HII regions
title_full An AST/RO Survey of CO(4-3) in ultracompact HII regions
title_fullStr An AST/RO Survey of CO(4-3) in ultracompact HII regions
title_full_unstemmed An AST/RO Survey of CO(4-3) in ultracompact HII regions
title_sort ast/ro survey of co(4-3) in ultracompact hii regions
publisher arXiv
publishDate 2003
url https://dx.doi.org/10.48550/arxiv.astro-ph/0306075
https://arxiv.org/abs/astro-ph/0306075
geographic Antarctic
The Antarctic
geographic_facet Antarctic
The Antarctic
genre Antarc*
Antarctic
genre_facet Antarc*
Antarctic
op_rights Assumed arXiv.org perpetual, non-exclusive license to distribute this article for submissions made before January 2004
http://arxiv.org/licenses/assumed-1991-2003/
op_doi https://doi.org/10.48550/arxiv.astro-ph/0306075
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