Extinction in star-forming disk galaxies from inclination-dependent composite spectra

Ching Wa Yip, Alex S. Szalay, Rosemary F G Wyse, Lszló Dobos, Tams Budavri, I. Csabai

Research output: Contribution to journalArticle

20 Citations (Scopus)

Abstract

Extinction in galaxies affects their observed properties. In scenarios describing the distribution of dust and stars in individual disk galaxies, the amplitude of the extinction can be modulated by the inclination of the galaxies. In this work, we investigate the inclination dependency in composite spectra of star-forming disk galaxies from the Sloan Digital Sky Survey Data Release 5. In a volume-limited sample within a redshift range 0.065-0.075 and a r-band Petrosian absolute magnitude range -19.5 to -22 mag which exhibits a flat distribution of inclination, the inclined relative to face-on extinction in the stellar continuum is found empirically to increase with inclination in the g, r, and i bands. Within the central 0.5 intrinsic half-light radius of the galaxies, the g-band relative extinction in the stellar continuum for the highly inclined objects (axis ratio b/a = 0.1) is 1.2 mag, agreeing with previous studies. The extinction curve of the disk galaxies is given in the rest-frame wavelengths 3700-8000, identified with major optical emission and absorption lines in diagnostics. The Balmer decrement, Hα/Hβ, remains constant with inclination, suggesting a different kind of dust configuration and/or reddening mechanism in the H II region from that in the stellar continuum. One factor is shown to be the presence of spatially non-uniform interstellar extinction, presumably caused by clumped dust in the vicinity of the H II region.

Original languageEnglish
Pages (from-to)780-790
Number of pages11
JournalAstrophysical Journal
Volume709
Issue number2
DOIs
Publication statusPublished - 2010

Fingerprint

disk galaxies
inclination
extinction
stars
composite materials
dust
H II regions
galaxies
continuums
interstellar extinction
light emission
optical absorption
radii
wavelength
curves
configurations
wavelengths

Keywords

  • Fundamental parameters
  • Methods: data analysis
  • Techniques: spectroscopic

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics
  • Nuclear and High Energy Physics

Cite this

Extinction in star-forming disk galaxies from inclination-dependent composite spectra. / Yip, Ching Wa; Szalay, Alex S.; Wyse, Rosemary F G; Dobos, Lszló; Budavri, Tams; Csabai, I.

In: Astrophysical Journal, Vol. 709, No. 2, 2010, p. 780-790.

Research output: Contribution to journalArticle

Yip, Ching Wa ; Szalay, Alex S. ; Wyse, Rosemary F G ; Dobos, Lszló ; Budavri, Tams ; Csabai, I. / Extinction in star-forming disk galaxies from inclination-dependent composite spectra. In: Astrophysical Journal. 2010 ; Vol. 709, No. 2. pp. 780-790.
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