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A&A 385, 1-13 (2002)
DOI: 10.1051/0004-6361:20020143
Chemically distinct nuclei and circumnuclear rings in lenticular galaxies NGC 4429 and NGC 7013
O. K. Sil'chenko1, 2, 3 and V. L. Afanasiev41 Sternberg Astronomical Institute, University Av. 13, Moscow 119899, Russia
2 Isaac Newton Institute of Chile, Moscow Branch
3 UK Astronomy Data Centre, Guest Investigator
4 Special Astrophysical Observatory, Nizhnij Arkhyz 369167, Russia
(Received 12 September 2001/ Accepted 13 December 2001 )
Abstract
The central regions of the regular lenticular galaxies
NGC 4429 and NGC 7013 have been studied with the Multi-Pupil
Field (Fiber) Spectrograph (MPFS) of the 6 m telescope of the
Special Astrophysical
Observatory RAS (Nizhnij Arkhyz, Russia) in two spectral ranges,
the blue one including the strong absorption lines
and
and the red one including the emission lines
H
and [
]
6583.
We confirm the presence of the chemically distinct nucleus
in NGC 7013 reported earlier. Besides this unresolved (in the
magnesium index) structure, we have found a ring of younger
stellar populations than those in the nucleus and in the bulge;
the radius of this ring is about 6´´ (400 pc). A similar
ring, distinguished by high magnesium- and iron-index values and
bordered by H
emission at its inner edge, with a radius
of 6´´ (500 pc), is found in NGC 4429. We try to relate the
ringed structure of the chemically decoupled cores in these galaxies
with past, now dissolved, large-scale bars whose remnants are
now seen in NGC 4429 and NGC 7013 as lenses between the bulges and
global disks. An analysis of the gas and star kinematics in the
centers of the galaxies has revealed the presence of an inclined
circumnuclear disk in NGC 7013 and the existence of minibar in
NGC 4429.
Key words: galaxies: individual: NGC 4429 -- galaxies: individual: NGC 7013 -- galaxies: nuclei -- galaxies: stellar content -- galaxies: kinematics and dynamics -- galaxies: evolution
Offprint request: O. K. Sil'chenko, olga@sai.msu.su
SIMBAD Objects
© ESO 2002
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