Astronomy and Astrophysics – Astrophysics
Scientific paper
2004-09-28
Astron.Astrophys. 429 (2005) 825-836
Astronomy and Astrophysics
Astrophysics
13 pages, 14 figures, accepted for publication in Astronomy and Astrophysics
Scientific paper
10.1051/0004-6361:20040311
The kinematics, structure, and stellar population properties in the centers of two early-type spiral galaxies of the Leo Triplet, NGC 3623 and NGC 3627, are studied by means of integral-field spectroscopy. Unlike our previous targets, NGC 3384/NGC 3368 in the Leo I group and NGC 5574/NGC 5576 in LGG379, NGC 3623 and NGC 3627 do not appear to experience a synchronous evolution. The mean ages of their circumnuclear stellar populations are quite different, and the magnesium overabundance of the nucleus in NGC 3627 is evidence for a very brief last star formation event 1 Gyr ago whereas the evolution of the central part of NGC 3623 looks more quiescent. In the center of NGC 3627 we observe noticeable gas radial motions, and the stars and the ionized gas in the center of NGC 3623 demonstrate more or less stable rotation. However, NGC 3623 has a chemically distinct core -- a relic of a past star formation burst -- which is shaped as a compact, dynamically cold stellar disk with a radius of about 250-350 pc which has been formed not later than 5 Gyr ago.
Afanasiev Victor L.
Sil'chenko Olga K.
No associations
LandOfFree
The Leo Triplet: Common origin or late encounter? 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 The Leo Triplet: Common origin or late encounter?, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Leo Triplet: Common origin or late encounter? will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-530391