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Dramatic Changes in Molecular Cloud Properties Across the Arp 299 Merger

Aalto, S. and Radford, S. J. E. and Scoville, N. Z. and Sargent, A. I. (1999) Dramatic Changes in Molecular Cloud Properties Across the Arp 299 Merger. In: Galaxy Interactions at Low and High Redshift. International Astronomical Union Symposium (IAUS). No.186. Springer , Dordrecht, pp. 231-234. ISBN 978-0-7923-5833-6. https://resolver.caltech.edu/CaltechAUTHORS:20190605-160239913

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Abstract

Arp 299 is an IR-luminous (L_(IR) ≈ 8 x 10^(11) L_⨀) merger system of two galaxies, IC 694 and NGC 3690, at a distance of 40 Mpc. Its proximity and richness in molecular gas make it suitable for studying the effects of gravitational interactions and starburst activity on molecular cloud distributions, dynamics, and physical conditions. Previous low resolution observations (10 – 30″) indicated that the CO/^(13)CO 1–0 intensity ratio is unusually high, > 20, suggesting an unusual population of molecular clouds (Aalto et al. 1991; Casoli et al. 1992).


Item Type:Book Section
Related URLs:
URLURL TypeDescription
https://doi.org/10.1007/978-94-011-4665-4_56DOIArticle
ORCID:
AuthorORCID
Scoville, N. Z.0000-0002-0438-3323
Sargent, A. I.0000-0002-4633-5098
Additional Information:© 1999 Springer Science+Business Media Dordrecht.
Series Name:International Astronomical Union Symposium (IAUS)
Issue or Number:186
Record Number:CaltechAUTHORS:20190605-160239913
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20190605-160239913
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:96175
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:06 Jun 2019 03:06
Last Modified:03 Oct 2019 21:19

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