Vicari, A. and Battinelli, P. and Capuzzo–Dolcetta, R. and Wyder, T. K. and Arrabito, G. (2002) Large-scale star formation in galaxies. II. The spirals NGC 3377A, NGC 3507 and NGC 4394. Young star groupings in spirals. Astronomy & Astrophysics, 384 (1). pp. 24-32. ISSN 0004-6361. doi:10.1051/0004-6361:20011803. https://resolver.caltech.edu/CaltechAUTHORS:20180226-081548304
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Abstract
The identification of young star groupings (YSG) in the three spiral galaxies NGC 3377A, NGC 3507, NGC 4394 is obtained by mean of the statistical method described in Paper I. We find 83, 90, 185 YSGs, respectively. An identification map of YSGs, as well as their size distribution, their B-luminosity function and their surface luminosity density radial behaviour are presented and compared. These data, in addition to those in Paper I, constitute a first sample suitable for seeking correlations among properties of galaxies and their YSGs, which we briefly discuss here.
Item Type: | Article | |||||||||
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Additional Information: | © 2002 ESO. Received: 28 June 2001. Accepted: 23 November 2001. | |||||||||
Subject Keywords: | galaxies: spiral - galaxies: general - galaxies: stellar content - stars: formation - methods: statistical | |||||||||
Issue or Number: | 1 | |||||||||
DOI: | 10.1051/0004-6361:20011803 | |||||||||
Record Number: | CaltechAUTHORS:20180226-081548304 | |||||||||
Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20180226-081548304 | |||||||||
Official Citation: | Large-scale star formation in galaxies - II. The spirals NGC 3377A, NGC 3507 and NGC 4394. Young star groupings in spirals A. Vicari, P. Battinelli, R. Capuzzo–Dolcetta, T. K. Wyder and G. Arrabito A&A, 384 1 (2002) 24-32 DOI: https://doi.org/10.1051/0004-6361:20011803 | |||||||||
Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | |||||||||
ID Code: | 84950 | |||||||||
Collection: | CaltechAUTHORS | |||||||||
Deposited By: | Ruth Sustaita | |||||||||
Deposited On: | 26 Feb 2018 19:34 | |||||||||
Last Modified: | 15 Nov 2021 20:24 |
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