Low-mass star formation in Lynds 1333
| Author | dc.contributor.author | Kun, M. | |
| Author | dc.contributor.author | Nikolić, Silvana | es_CL |
| Author | dc.contributor.author | Johansson, L. E. B. | es_CL |
| Author | dc.contributor.author | Balog, Z. | es_CL |
| Author | dc.contributor.author | Gáspár, A. | es_CL |
| Admission date | dc.date.accessioned | 2009-04-14T15:31:01Z | |
| Available date | dc.date.available | 2009-04-14T15:31:01Z | |
| Publication date | dc.date.issued | 2006-09-11 | |
| Cita de ítem | dc.identifier.citation | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY Volume: 371 Issue: 2 Pages: 732-738 Published: SEP 11 2006 | en |
| Identifier | dc.identifier.issn | 0035-8711 | |
| Identifier | dc.identifier.uri | https://repositorio.uchile.cl/handle/2250/124902 | |
| Abstract | dc.description.abstract | Medium-resolution optical spectroscopy of the candidate young stellar objects associated with the small, nearby molecular cloud Lynds 1333 revealed four previously unknown classical T Tauri stars, two of which are components of a visual double, and a Class I source, IRAS 02086+7600. The spectroscopic data, together with new V, R-C, I-C photometric and 2MASS J, H, and K-s data allowed us to estimate the masses and ages of the new T Tauri stars. We touch on the possible scenario of star formation in the region. L 1333 is one of the smallest and nearest known star-forming clouds, therefore it may be a suitable target for studying in detail the small-scale structure of a star-forming environment. | en |
| Lenguage | dc.language.iso | en | en |
| Publisher | dc.publisher | BLACKWELL | en |
| Keywords | dc.subject | T-TAURI STARS | en |
| Título | dc.title | Low-mass star formation in Lynds 1333 | en |
| Document type | dc.type | Artículo de revista |
Files in this item
This item appears in the following Collection(s)
-
Artículos de revistas
Artículos de revistas