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Nascent Starbursts in Synchrotron-Deficient Galaxies

Roussel, Hélène and Helou, George and Condon, James and Beck, Rainer (2005) Nascent Starbursts in Synchrotron-Deficient Galaxies. In: Starbursts: From 30 Doradus to Lyman Break Galaxies. Astrophysics and Space Science Library. No.329. Springer Netherlands , Dordrecht, pp. 223-226. ISBN 978-1-4020-3538-8. https://resolver.caltech.edu/CaltechAUTHORS:20201014-150720595

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Abstract

We have identified a rare category of galaxies deviating from the universal infrared-radio correlation of star-forming galaxies in being significantly deficient in synchrotron radiation at 20 cm. The selected objects also have high dust temperatures, indicating intense radiation fields. From a detailed study of the prototype of this class, NGC 1377, the most likely scenario accounting for their properties is a starburst just breaking out in a host previously quiescent for at least 100 Myr. We have selected a statistical sample of candidate nascent starbursts from the cross-correlation of the IRAS Faint Source Catalog with the NVSS and FIRST VLA radio surveys, and discuss the first results obtained from a recent multi-wavelength VLA campaign.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
https://doi.org/10.1007/1-4020-3539-x_39DOIArticle
https://rdcu.be/b8wyBPublisherFree ReadCube access
ORCID:
AuthorORCID
Helou, George0000-0003-3367-3415
Condon, James0000-0003-4724-1939
Additional Information:© 2005 Springer.
Group:Infrared Processing and Analysis Center (IPAC)
Subject Keywords:Dust Temperature; Rare Category; Young Stellar Population; Star Burst; Cent Imeter Wave
Series Name:Astrophysics and Space Science Library
Issue or Number:329
DOI:10.1007/1-4020-3539-x_39
Record Number:CaltechAUTHORS:20201014-150720595
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20201014-150720595
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:106071
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:14 Oct 2020 22:27
Last Modified:16 Nov 2021 18:49

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