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Published January 14, 2014 | public
Book Section - Chapter

Mapping the Star Formation in Orion A/L1641

Abstract

First phases of the process of star formation are characterized by excess in infrared and high X-ray emission. With Spitzer and XMM-Newton we have surveyed the Orion A part relative to the filamentary cloud Lynds 1641 (L1641). Furthermore, an extended spectroscopic survey has been realized to better constraint the cluster membership of stars without IR excess.

Additional Information

© 2014 Springer.

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August 19, 2023
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January 13, 2024