Addendum: An Investigation into the Prominence of Spiral Galaxy Bulges [Astron. J. [URL ADDRESS="/cgi-bin/resolve?2001AJ....121..820G" STATUS="OKAY"]121, 820[/URL]; [URL ADDRESS="/cgi-bin/resolve?2001AJ....122.1067G" STATUS="OKAY"]122, 1067[/URL] (2001)] | Zendy

Alister W. Graham | Zendy

Open Access

Addendum: An Investigation into the Prominence of Spiral Galaxy Bulges [Astron. J. [URL ADDRESS="/cgi-bin/resolve?2001AJ....121..820G" STATUS="OKAY"]121, 820[/URL]; [URL ADDRESS="/cgi-bin/resolve?2001AJ....122.1067G" STATUS="OKAY"]122, 1067[/URL] (2001)]

Author(s) -

Alister W. Graham

Publication year - 2003

Publication title -

the astronomical journal

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 2.61

H-Index - 271

eISSN - 1538-3881

pISSN - 0004-6256

DOI - 10.1086/375000

Subject(s) - astrophysics , bulge , bin , physics , galaxy , spiral galaxy , spiral (railway) , astron , homogeneous , computer science , statistical physics , mathematics , algorithm , mathematical analysis

The best-fitting B, R, I and K-band (Sersic R^(1/n) bulge + exponential disk)model parameters for the de Jong & van der Kruit (1994) sample of 86 spiralgalaxies are made electronically available. This sample covers all spiralgalaxy types and provides the largest homogeneous set of structural parametersfor spiral galaxies modeled with an R^(1/n) bulge.Comment: An Addendum to appear in AJ. Readers are welcome to request ascii tables and/or diagrams of the fitted profiles from the Autho

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