Astronomy and Astrophysics – Astrophysics
Scientific paper
May 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996a%26as..116..515r&link_type=abstract
Astronomy and Astrophysics Supplement, v.116, p.515-571
Astronomy and Astrophysics
Astrophysics
26
Galaxies: Photometry, Galaxies: Elliptical And Lenticular, Galaxies: Spiral, Galaxies: Interactions, Galaxies: Evolution
Scientific paper
We present the multicolour (B, V, R) surface photometry of 53 double galaxies. All the pairs belong to the catalogue of Reduzzi & Rampazzo (1995) containing objects selected according to the Karachentsev (1972) criteria. We comment on the morphological, structural and photometric characteristics of pairs and their members. Different classes of interaction induced phenomena, both among early and late-type galaxies, are considered. We found that few early-type galaxies show fine structures. Grand design structure is more frequently detected in binary than in field spirals both for barred and non barred, confirming Elmegreen & Elmegreen's (1982) study. The colour of the tails is consistent with the stripping hypothesis since it is similar to the progenitor galaxy outskirts. Among our objects we have no evident sign of induced star formation in tails. Rings appear on average bluer than the disc as a whole.
Rampazzo Roberto
Reduzzi Luca
No associations
LandOfFree
Surface photometry of binary galaxies. I. A multicolour study of morphologies due to the interaction. does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Surface photometry of binary galaxies. I. A multicolour study of morphologies due to the interaction., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Surface photometry of binary galaxies. I. A multicolour study of morphologies due to the interaction. will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1351616