Abstract
As a region of recent star formation and intense stellar activity the Orion Complex extending over several square degrees is of paramount importance in the study of early evolution and activity in the stellar chromospheres of low mass stars. Although red stars form a rather inhomogeneous group, including foreground K-M dwarfs, distant K-M giants, carbon stars and a variety of reddened objects, in principle these can be separated from a combination of photometric, spectroscopic and kinematic data. The proximity of the Orion Complex and its relatively high galactic latitude mean that future astrometric and radial velocity work will yield useful kinematical information on all member stars, including the enigmatic pre-main sequence stars on the lower part of the HR diagram. For these stars, differences in spectroscopic properties, photometric behaviour, kinematics and the interstellar environment contain the key to some of the problems, presently insurmountable, in the early evolution of the entire Orion Complex.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Preview
Unable to display preview. Download preview PDF.
References
Andrews, A.D., 1981 ‘A Photometric Atlas of the Orion Nebula’, published at Armagh Observatory.
Kutner, M.L., Tucker, K.D., Chin, G. and Thaddeus, P., 1977 Astrophys. Journ. 215, pp.521–528.
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1984 D. Reidei Publishing Company
About this paper
Cite this paper
Andrews, A.D., McGee, B. (1984). Use of the UK Schmidt for a Photometric Investigation of Red Stars in the Orion Nebula Molecular Complex. In: Capaccioli, M. (eds) Astronomy with Schmidt-Type Telescopes. Astrophysics and Space Science Library, vol 110. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-6387-0_46
Download citation
DOI: https://doi.org/10.1007/978-94-009-6387-0_46
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-009-6389-4
Online ISBN: 978-94-009-6387-0
eBook Packages: Springer Book Archive