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2001MNRAS.327..385S - Mon. Not. R. Astron. Soc., 327, 385-396 (2001/October-3)
The energetics and mass loss of the dwarf starburst Markarian 33.
SUMMERS L.K., STEVENS I.R. and STRICKLAND D.K.
Abstract (from CDS):
We estimate the age and mass of Mrk 33's starburst to be 5.8Myr and 6.9.106Msolar respectively, with the energy injection rate in the central regions of the galaxy being ∼1041ergs–1, while the associated mass-loss rate from the star-forming regions is estimated to be ∼0.2M☉yr–1. We suggest that the X-ray emission is predominantly powered by starburst-type activity, and argue that a blow-out in the form of a galactic wind is the most likely fate for Mrk 33, resulting in the loss of most of the galaxy's metal-enriched material and a small fraction (<1 per cent) of the ISM.
Abstract Copyright: The Royal Astronomical Society
Journal keyword(s): stars: Wolf-Rayet - ISM: jets and outflows - galaxies: individual: Mrk 33 - galaxies: starburst - galaxies: stellar content - X-rays: galaxies
Nomenclature: Fig.2: [SSS2001] Mrk 33 W (Nos N, S). Fig.1, Table A1: [SSS2001] X-NN (Nos X-1 to X-23).
Simbad objects: 30
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