Spectrophotometric investigations of the blue compact dwarf galaxy Mrk 35

Details Spectrophotometric investigations of the blue compact dwarf galaxy Mrk 35 Spectrophotometric investigations of the blue compact dwarf galaxy Mrk 35

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003ap%26ss.284..611c&link_type=abstract

Astrophysics and Space Science, v. 284, Issue 2, p. 611-614 (2003).

Astronomy and Astrophysics

Astrophysics

2

Galaxies: Individual(Markarian 35), Galaxies: Starburst, Galaxies: Structure

Scientific paper

Preliminary results from a detailed spectrophotometric analysis of the blue compact dwarf galaxy (BCD) Mrk 35 are presented. We have performed deep UBVRI broad-band and Hα narrow-band optical observations, near-infrared (JHK s) imaging and long-slit spectroscopy of the galaxy. Mrk 35 is composed of a very young starburst population distributed in a bar-like structure, placed on top of an underlying, older stellar host galaxy. Using predictions of evolutionary synthesis models, we estimate the ages of both the starburst regions and the underlying stellar component.

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