Mapping the Star Formation in Orion A/L1641

Pillitteri, Ignazio; Wolk, S. J.; Megeath, S. T.; Allen, L.; Bally, J.; Gagné, Marc; Gutermuth, R. A.; Hartman, L.; Micela, G.; Myers, P.; Oliveira, J. M.; Sciortino, S.; Walter, F.; Rebull, L.; Stauffer, J.

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. We find that:

Citation

Pillitteri, I., Wolk, S. J., Megeath, S. T., Allen, L., Bally, J., Gagné, M., …Stauffer, J. (2014). Mapping the Star Formation in Orion A/L1641. In The Labyrinth of Star Formation (291-293). https://doi.org/10.1007/978-3-319-03041-8_56

• Conference Name: The Labyrinth of Star Formation
• Conference Location: Crete, Greece
• Online Publication Date: Jan 1, 2014
• Publication Date: Apr 16, 2014
• Deposit Date: Jun 16, 2023
• Publisher: Springer
• Pages: 291-293
• Series Title: Astrophysics and Space Science Proceedings
• Series ISSN: 1570-6591
• Book Title: The Labyrinth of Star Formation
• ISBN: 9783319030401; 9783319030418
• DOI: https://doi.org/10.1007/978-3-319-03041-8_56
• Keywords: Star Formation Cluster Membership Iota Orionis Young Stellar Population Cloud Filament
• Additional Information: First Online: 28 January 2014