Two-dimensional decomposition of bulge and disk

Y. I. Byun, K. C. Freeman

Research output: Contribution to journalArticle

78 Citations (Scopus)

Abstract

We describe a method of bulge-to-disk decomposition which utilizes a full two-dimensional image of a galaxy. It provides much better estimates of the structural parameters for each component than the widely used conventional procedure which involves a X2 decomposition on elliptically averaged profiles. The performances of the conventional one-dimensional method and the present two-dimensional technique are compared by using a set of realistic model galaxy images. We show that the conventional one-dimensional decomposition procedure is subject to strong systematic errors associated with the derivation of the elliptically averaged radial surface brightness profiles; these errors come from the different intrinsic shapes of disk and bulge, combined with the effects of viewing inclination. The present two-dimensional approach successfully recovers the intrinsic parameters for a wide range of B/D ratios at all inclinations.

Original languageEnglish
Pages (from-to)563-574
Number of pages12
JournalAstrophysical Journal
Volume448
Issue number2
DOIs
Publication statusPublished - 1995 Aug 1

Fingerprint

decomposition
inclination
galaxies
profiles
systematic errors
brightness
derivation
estimates
parameter
method
effect

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Byun, Y. I. ; Freeman, K. C. / Two-dimensional decomposition of bulge and disk. In: Astrophysical Journal. 1995 ; Vol. 448, No. 2. pp. 563-574.
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Two-dimensional decomposition of bulge and disk. / Byun, Y. I.; Freeman, K. C.

In: Astrophysical Journal, Vol. 448, No. 2, 01.08.1995, p. 563-574.

Research output: Contribution to journalArticle

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