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 language | English (US) |
|---|---|
| Pages (from-to) | 434-438 |
| Number of pages | 5 |
| Journal | Baltic Astronomy |
| Volume | 13 |
| Issue number | 3 |
| State | Published - 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