The Relation Between Field Massive Stars and Clusters
| Autor: | J. B. Lamb, J. Wm. Parker, M. S. Oey, N. L. King |
|---|---|
| Rok vydání: | 2007 |
| Předmět: |
Physics
Spiral galaxy K-type main-sequence star Stellar collision Astronomy Astronomy and Astrophysics Astrophysics::Cosmology and Extragalactic Astrophysics Astrophysics Blue straggler Stars T Tauri star Star cluster Space and Planetary Science Astrophysics::Solar and Stellar Astrophysics Astrophysics::Earth and Planetary Astrophysics Astrophysics::Galaxy Astrophysics Open cluster |
| Zdroj: | Proceedings of the International Astronomical Union. 3:65-66 |
| ISSN: | 1743-9221 1743-9213 |
| DOI: | 10.1017/s1743921308015305 |
| Popis: | Massive “field” stars are those that appear in apparent isolation, in contrast to those in clusters. Whereas cluster stars are formed together in large aggregates, simultaneously, field stars have multiple origins. Some massive field stars may be the “tip of the iceberg” on small groups of physically associated stars, while others appear to be “runaway” stars that are dynamically ejected from clusters. What is the intrinsic relation between clusters and field stars, and what is the faction of runaway stars? Since massive stars are the most luminous stellar population, their demographics are accessible in the nearest external galaxies. We present our current efforts to understand these issues for the Small Magellanic Cloud. |
| Databáze: | OpenAIRE |
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