CaltechAUTHORS
Published January 14, 2014 | Version public
Book Section - Chapter Metadata-only

Mapping the Star Formation in Orion A/L1641

Creators

  • 1. ROR icon Smithsonian Astrophysical Observatory
  • 2. ROR icon University of Toledo
  • 3. ROR icon NOIRLab
  • 4. ROR icon University of Colorado Boulder
  • 5. ROR icon West Chester University
  • 6. ROR icon University of Massachusetts Amherst
  • 7. ROR icon University of Michigan–Ann Arbor
  • 8. ROR icon Osservatorio Astronomico di Palermo
  • 9. ROR icon Keele University
  • 10. ROR icon California Institute of Technology

Contributors

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.

Additional details

Identifiers

Eprint ID
79205
DOI
10.1007/978-3-319-03041-8_56
Resolver ID
CaltechAUTHORS:20170719-110502897

Dates

Created
2017-07-19
Created from EPrint's datestamp field
Updated
2021-11-15
Created from EPrint's last_modified field

Caltech Custom Metadata

Caltech groups
Physics Department
Series Name
Astrophysics and Space Science Proceedings
Series Volume or Issue Number
36