Mapping the Star Formation in Orion A/L1641

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

Others:: Stamatellos, D.; Goodwin, S.; Ward-Thompson, D.

Style

An error occurred while generating the citation.

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.

	All versions	This version
Views	0	0
Downloads	0	0
Data volume	0 Bytes	0 Bytes

Mapping the Star Formation in Orion A/L1641

Abstract

Additional Information

Additional details