Hostname: page-component-7bb8b95d7b-2h6rp Total loading time: 0 Render date: 2024-09-12T13:21:33.216Z Has data issue: false hasContentIssue false

Age Spread of the Orion Nebular Stars

Published online by Cambridge University Press:  14 August 2015

Syuzo Isobe
Affiliation:
Tokyo Astronomical Observatory, University of Tokyo, 2-21-1, Osawa, Mitaka, Tokyo, Japan, 181
Goro Sasaki
Affiliation:
Tokyo Astronomical Observatory, University of Tokyo, 2-21-1, Osawa, Mitaka, Tokyo, Japan, 181

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The Orion Nebula is a recent star formation place on a sequence of star formation in the Orion Association Ia to Id and further to the Orion Molecular cloud as shown by Kutner, Tucker, Chin, and Thaddeus (1977). From the photoelectric observations, Penston (1973, 1975) obtained the age of the Nebula younger than 3×106 years.

Type
Session 2: Pre-Main-Sequence Evolution and Formation of Binary Stars
Copyright
Copyright © Reidel 1981