Far-infrared luminosity functions of normal galaxies

Takashi Isobe, Eric D. Feigelson

Research output: Contribution to journalArticle

30 Citations (Scopus)

Abstract

A volume-limited sample (≤ 1400 km s-1; corrected for local motion) is constructed from the Zwicky catalog and IRAS data base to examine the far-infrared (FIR) luminosity functions of normal galaxies, and to investigate possible relationships between FIR emission and galaxy morphology. Quantitative and unbiased treatment is provided by "survival analysis" statistical methods. We find that the FIR distributions of normal galaxies are better fit by lognormal than Schechter functions. The total FIR emissivity (8 to 115 μm) of normal galaxies is approximately equal to half their emission in the B plus V optical bands. Normal galaxy FIR emission is uncorre-lated with the basic S0-Sm Hubble sequence of spiral galaxy morphology, but appears to be affected by de Vaucouleurs' revised morphological classifications based on inner rings and S-shaped arms. Spirals with bars and inner rings are systematically fainter than unbarred spirals. We suggest that bars and rings reduce the amount or spatially confine the dust in spiral disks, resulting in lower efficiency conversion of optical and UV photons into the infrared.

Original languageEnglish (US)
Pages (from-to)197-211
Number of pages15
JournalAstrophysical Journal, Supplement Series
Volume79
Issue number2
DOIs
StatePublished - Apr 1992

Fingerprint

luminosity
galaxies
emissivity
rings
statistical analysis
dust
data bases
Infrared Astronomy Satellite
spiral galaxies
catalogs
photons
distribution
method
data base

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

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Far-infrared luminosity functions of normal galaxies. / Isobe, Takashi; Feigelson, Eric D.

In: Astrophysical Journal, Supplement Series, Vol. 79, No. 2, 04.1992, p. 197-211.

Research output: Contribution to journalArticle

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AU - Feigelson, Eric D.

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