Ambipolar-diffusion timescale, star formation timescale, and the ages of molecular clouds: Is there a discrepancy?

Konstantinos Tassis, Telemachos Ch Mouschovias

Research output: Contribution to journalArticle

Abstract

We reexamine critically the estimates of the duration of different phases of star formation and the lifetimes of molecular clouds based on the ages of T Tauri stars, age spreads of stars in clusters, and statistics of prestellar cores. We show that all available observational data are consistent with lifetimes of molecular clouds comparable to ∼107 yr, as well as with the predictions of the theory of self-initiated, ambipolar-diffusion-controlled star formation. We conclude that there exists no observational support for either "young" molecular clouds or "rapid" star formation.

Original languageEnglish (US)
Pages (from-to)283-287
Number of pages5
JournalAstrophysical Journal
Volume616
Issue number1 I
DOIs
StatePublished - Nov 20 2004

Keywords

  • Accretion, accretion disks
  • Dust, extinction
  • ISM: Magnetic fields MHD
  • ISM: clouds
  • Stars: formation

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Fingerprint Dive into the research topics of 'Ambipolar-diffusion timescale, star formation timescale, and the ages of molecular clouds: Is there a discrepancy?'. Together they form a unique fingerprint.

  • Cite this