Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4605
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dc.contributor.authorRamya, S-
dc.contributor.authorSahu, D. K-
dc.contributor.authorPrabhu, T. P-
dc.date.accessioned2009-07-01T10:17:24Z-
dc.date.available2009-07-01T10:17:24Z-
dc.date.issued2009-06-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, Vol. 396, No. 1, pp. 97 - 108en
dc.identifier.issn0035-8711-
dc.identifier.urihttp://hdl.handle.net/2248/4605-
dc.description.abstractTwo blue compact dwarf galaxies, Mkn 104 and I Zw 97, are studied photometrically and spectroscopically. Mkn 104 is found to contain three distinct bright star-forming regions, whereas I Zw 97 is found to contain three bright and two faint star-forming regions. Medium-resolution spectra of three bright HII regions in the two galaxies were obtained. Estimation of oxygen abundance in these regions yields a value equal to log(O/H) + 12 = 8.5 (Z = Zsolar/2.7). Star-formation rates in these star-forming regions are estimated. The highest star-formation rate for I Zw 97 is found to be 0.04Msolaryr-1, and for Mkn 104 it is 0.02Msolaryr-1. I Zw 97 is realized to be a cometary blue compact dwarf galaxy undergoing a strong burst of star formation. A U - B versus V - I colour-colour mixed population model is created using the Starburst99 evolutionary model curves. The spectrum of the bright star-forming knot of I Zw 97 does not show any strong signature of an underlying relatively older stellar population, but the U - B versus V - I two-colour diagram indicates the strong contribution of a ~500Myr population. A spectrum of the central region of Mkn 104 gives a hint about the underlying old stellar population. The age of this underlying population using the U - B versus V - I two-colour diagram is estimated to be ~ 500Myr. Surface-brightness profiles and colour profiles for these galaxies are presented. The surface-brightness profile of both the galaxies can be represented well by a two-component Sérsic profile consisting of a near-exponential distribution and a Gaussian nuclear starburst. To conclude, neither of these galaxies is a young system; instead they are undergoing episodic star formation superposed on a faint older component. I Zw 97 is a cometary blue compact dwarf galaxy where the underlying low-surface-brightness (LSB) galaxy is a dwarf irregular observed during a major stochastic enhancement of its otherwise moderate star-formation activity, a phenomenon widely accepted as self-propagating stochastic star formation. Both of these galaxies are very similar in their stellar content, showing an older 4-Gyr population, an intermediate 500-Myr population and the current burst of star formation of age 5-13 Myr.en
dc.language.isoenen
dc.publisherBlackwell Publishingen
dc.relation.urihttp://dx.doi.org/10.1111/j.1365-2966.2009.14731.xen
dc.rights© Royal Astronomical Societyen
dc.subjectTechniques: photometricen
dc.subjectGalaxies: individual: I Zw 97en
dc.subjectGalaxies: individual: Mkn 104en
dc.subjectGalaxies: starbursten
dc.titleStar formation in blue compact dwarf galaxies: Mkn 104 and I Zw 97en
dc.typeArticleen
Appears in Collections:IIAP Publications
Publications based on data from IAO, Hanle

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