Multiplicity of the massive stars in the Orion Nebula cluster
- 1 December 1999
- journal article
- Published by Elsevier in New Astronomy
- Vol. 4 (7) , 531-542
- https://doi.org/10.1016/s1384-1076(99)00042-1
Abstract
No abstract availableKeywords
This publication has 33 references indexed in Scilit:
- The Stellar Initial Mass Function from Random Sampling in Hierarchical Clouds. II. Statistical Fluctuations and a Mass Dependence for Starbirth Positions and TimesThe Astrophysical Journal, 1999
- On the formation of massive starsMonthly Notices of the Royal Astronomical Society, 1998
- Externally Illuminated Young Stellar Environments in the Orion Nebula: [ITAL]Hubble[/ITAL] [ITAL]Space[/ITAL] [ITAL]Telescope[/ITAL] Planetary Camera and Ultraviolet ObservationsThe Astronomical Journal, 1998
- On the Periodic X-Ray Emission from θ[TSUP]1[/TSUP] Orionis CThe Astrophysical Journal, 1997
- Astrostatistics.Published by JSTOR ,1996
- New pre-main-sequence tracks for M less than or equal to 2.5 solar mass as tests of opacities and convection modelThe Astrophysical Journal Supplement Series, 1994
- Spectroscopic binaries in the Orion Nebula clusterThe Astrophysical Journal, 1991
- The frequency and formation mechanism of B2-B5 main-sequence binariesThe Astrophysical Journal Supplement Series, 1990
- Normal and Abnormal Binary FrequenciesAnnual Review of Astronomy and Astrophysics, 1983
- Binaries among B2-B5 IV, V absorption and emission starsThe Astrophysical Journal Supplement Series, 1978