On the evolutionary history of stars and their fossil mass and light

Mark A. Fardal, Neal Katz, David H. Weinberg, Romeel S Dave

Research output: Contribution to journalArticle

94 Citations (Scopus)

Abstract

The total extragalactic background radiation can be an important test of the global star formation history (SFH). Using direct observational estimates of the SFH, along with standard assumptions about the initial mass function (IMF), we calculate the total extragalactic background radiation and the observed stellar density today. We show that plausible SFHs allow a significant range in each quantity, but that their ratio is very tightly constrained. Current estimates of the stellar mass and extragalactic background are difficult to reconcile, as long as the IMF is fixed to the Salpeter slope above 1 M⊙. The joint confidence interval of these two quantities only agrees with that determined from the allowed range of SFH fits at the 3σ level, and for our best-fitting values the discrepancy is about a factor of 2. Alternative energy sources that contribute to the background, such as active galactic nuclei (AGN), Population III stars or decaying particles, appear unlikely to resolve the discrepancy. However, changes to the IMF allow plausible solutions to the background problem. The simplest is an average IMF with an increased contribution from stars around 1.5-4 M⊙. A 'paunchy' IMF of this sort could emerge as a global average if low-mass star formation is suppressed in galaxies experiencing rapid starbursts. Such an IMF is consistent with observations of star-forming regions, and would help to reconcile the fossil record of star formation with the directly observed SFH.

Original languageEnglish (US)
Pages (from-to)985-1002
Number of pages18
JournalMonthly Notices of the Royal Astronomical Society
Volume379
Issue number3
DOIs
StatePublished - Aug 2007

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fossils
star formation
histories
fossil
stars
history
background radiation
Population III stars
energy sources
estimates
alternative energy
stellar mass
active galactic nuclei
fossil record
confidence
confidence interval
slopes
galaxies
intervals

Keywords

  • Diffuse radiation
  • Galaxies: stellar content

ASJC Scopus subject areas

  • Space and Planetary Science

Cite this

On the evolutionary history of stars and their fossil mass and light. / Fardal, Mark A.; Katz, Neal; Weinberg, David H.; Dave, Romeel S.

In: Monthly Notices of the Royal Astronomical Society, Vol. 379, No. 3, 08.2007, p. 985-1002.

Research output: Contribution to journalArticle

Fardal, Mark A. ; Katz, Neal ; Weinberg, David H. ; Dave, Romeel S. / On the evolutionary history of stars and their fossil mass and light. In: Monthly Notices of the Royal Astronomical Society. 2007 ; Vol. 379, No. 3. pp. 985-1002.
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