Infrared emission of young HII regions: A Herschel /Hi-GAL study

Cesaroni, Riccardo, Pestalozzi, Michele R., Beltrán, Maria T., Hoare, Michael G., Molinari, Sergio, Olmi, Luca, Smith, Michael D., Stringfellow, Guy S., Testi, Leonardo, Thompson, Mark A. and others. (2015) Infrared emission of young HII regions: A Herschel /Hi-GAL study. Astronomy & Astrophysics, 579 . p. 25953. ISSN 0004-6361. (doi:10.1051/0004-6361/201525953) (The full text of this publication is not currently available from this repository. You may be able to access a copy if URLs are provided) (KAR id:50078)

The full text of this publication is not currently available from this repository. You may be able to access a copy if URLs are provided.
Official URL: http://www.dx.doi.org/10.1051/0004-6361/201525953

Abstract

Context. Investigating the relationship between radio and infrared emission of Hii regions may help shed light on the nature of the ionizing stars and the formation mechanism of early-type stars in general.

Aims. We have taken advantage of recent unbiased surveys of the Galactic plane such as Herschel/Hi-GAL and VLA/CORNISH to study a bona fide sample of young Hii regions located in the Galactic longitude range 10°–65° by comparing the mid- and far-IR continuum emission to the radio free-free emission at 5 GHz.

Item Type:	Article
DOI/Identification number:	10.1051/0004-6361/201525953
Uncontrolled keywords:	stars ; early-type ; formation ; Hiiregions
Subjects:	Q Science > QB Astronomy > QB460 Astrophysics
Divisions:	Divisions > Division of Natural Sciences > Physics and Astronomy
Depositing User:	Giles Tarver
Date Deposited:	10 Aug 2015 15:39 UTC
Last Modified:	17 Aug 2022 10:59 UTC
Resource URI:	https://kar.kent.ac.uk/id/eprint/50078 (The current URI for this page, for reference purposes)

University of Kent Author Information

Smith, Michael D..

Creator's ORCID:	https://orcid.org/0000-0002-4289-5952
CReDIT Contributor Roles:

Thompson, Mark A..

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