Initial conditions of low, intermediate and high mass star formation

M. Kun, D. Apai, I. 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
Pages (from-to)434-438
Number of pages5
JournalBaltic Astronomy
Volume13
Issue number3
Publication statusPublished - Jan 1 2004

Keywords

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

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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  • Cite this

    Kun, M., Apai, D., Pascucci, I., Nikolić, S., & Eredics, M. (2004). Initial conditions of low, intermediate and high mass star formation. Baltic Astronomy, 13(3), 434-438.