Large scale star formation in galaxies. II. The spirals NGC 3377A, NGC 3507 and NGC 4394

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dc.creatorVicari, A.
dc.creatorBattinelli, P.
dc.creatorCapuzzo--Dolcetta, R.
dc.creatorWyder, T. K.
dc.creatorArrabito, G.
dc.date2001-07-05
dc.date2001-10-29
dc.date.accessioned2026-07-07T01:59:11Z
dc.date.available2026-07-07T01:59:11Z
dc.descriptionThe 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, their surface luminosity density radial behaviour, are presented and comparatively discussed. These data, in addition to those in Paper I, constitute a first sample suitable for seeking correlations among properties of galaxies and their YSG, which we briefly discuss here.
dc.descriptionin press in A&A; 15 pages including 7 figures and 3 tables
dc.identifierhttps://arxiv.org/abs/astro-ph/0107100
dc.identifierhttp://arxiv.org/abs/astro-ph/0107100
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/3012
dc.subjectAstrophysics
dc.titleLarge scale star formation in galaxies. II. The spirals NGC 3377A, NGC 3507 and NGC 4394
dc.typetext

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