Initial conditions of low, intermediate and high mass star formation

M. Kun, Daniel Apai, Ilaria Pascucci, S. Nikolić, M. Eredics

Research output: Contribution to journalArticle

Abstract

We examined the structures and star-forming properties of three nearby molecular clouds, usually not included in star formation studies: the small filamentary complex L1333, the cometary-shaped cloud L1251, and L1340, a round fragmented cloud forming moderate size clusters of low- and intermediate-mass stars. We compare some properties of these clouds with other nearby regions of low- and high-mass star formation.

Original languageEnglish (US)
Pages (from-to)434-438
Number of pages5
JournalBaltic Astronomy
Volume13
Issue number3
StatePublished - 2004
Externally publishedYes

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star formation
stars
molecular clouds

Keywords

  • Ism: clouds: individual (L 1251, L 1333, L 1340)
  • Stars: formation
  • Stars: pre-main-sequence

ASJC Scopus subject areas

  • Astronomy and Astrophysics

Cite this

Initial conditions of low, intermediate and high mass star formation. / Kun, M.; Apai, Daniel; Pascucci, Ilaria; Nikolić, S.; Eredics, M.

In: Baltic Astronomy, Vol. 13, No. 3, 2004, p. 434-438.

Research output: Contribution to journalArticle

Kun, M, Apai, D, Pascucci, I, Nikolić, S & Eredics, M 2004, 'Initial conditions of low, intermediate and high mass star formation', Baltic Astronomy, vol. 13, no. 3, pp. 434-438.
Kun, M. ; Apai, Daniel ; Pascucci, Ilaria ; Nikolić, S. ; Eredics, M. / Initial conditions of low, intermediate and high mass star formation. In: Baltic Astronomy. 2004 ; Vol. 13, No. 3. pp. 434-438.
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