The anomalous properties of Markarian 1460

Trentham, Neil; Tully, Brent R.; Verheijen, M.A.W.

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1499

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DC Field	Value	Language
dc.contributor.author	Trentham, Neil	-
dc.contributor.author	Tully, Brent R.	-
dc.contributor.author	Verheijen, M.A.W.	-
dc.date.accessioned	2006-11-04T11:08:54Z	-
dc.date.available	2006-11-04T11:08:54Z	-
dc.date.issued	2001-08	-
dc.identifier.citation	Monthly Notices of the Royal Astronomical Society, 2001, Vol.325, p1275-1280	en
dc.identifier.issn	0035-8711	-
dc.identifier.uri	http://hdl.handle.net/2289/1499	-
dc.description	Open Access	en
dc.description.abstract	We present and discuss optical, near-infrared and H i measurements of the galaxy Markarian 1460 at a distance of 19 Mpc in the Ursa Major Cluster. This low-luminosity (MB=−14) galaxy is unusual because (i) it is blue (B−R=0.8) and has the spectrum of an H ii galaxy, (ii) it has a light profile that is smooth and well fitted by an r1/4 and not an exponential function at all radii larger than the seeing, and (iii) it has an observed central brightness of about μB=20 mag arcsec-2, intermediate between those of elliptical galaxies (on the bright μB side) and normal low-luminosity dwarf irregular (on the low μB side) galaxies. No other known galaxy exhibits all these properties in conjunction. On morphological grounds this galaxy looks like a normal distant luminous elliptical galaxy, since the Fundamental Plane tells us that higher luminosity normal elliptical galaxies tend to have lower surface-brightnesses. Markarian 1460 has 2×107 Mo of H i and a ratio M(H i)/LB of 0.2, which is low compared to the typical values for star-forming dwarf galaxies. From the high surface-brightness and r1/4 profile, we infer that the baryonic component of Markarian 1460 has become self-gravitating through dissipative processes. From the colours, radio continuum, H i and optical emission line properties, and yet smooth texture, we infer that Markarian 1460 has had significant star formation as recently as ~1 Gyr ago but not today.	en
dc.format.extent	8338 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Blackwell Publishing for the Royal Astronomical Society	en
dc.relation.uri	http://adsabs.harvard.edu/cgi-bin/bib_query?2001MNRAS.325.1275T	en
dc.relation.uri	http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?2001MNRAS.325.1275T&data_type=PDF_HIGH&type=PRINTER&filetype=.pdf	en
dc.rights	(2001) Royal Astronomical Society	en
dc.subject	GALAXIES: CLUSTERS: INDIVIDUAL: URSA MAJOR	en
dc.subject	GALAXIES: INDIVIDUAL: MARKARIAN 1460	en
dc.subject	GALAXIES: PHOTOMETRY	en
dc.title	The anomalous properties of Markarian 1460	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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