Infrared Spectra of Young Stars Embedded in the R Coronae Australis Cloud

Details Infrared Spectra of Young Stars Embedded in the R Coronae Australis Cloud Infrared Spectra of Young Stars Embedded in the R Coronae Australis Cloud

Apr 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009pasp..121..350m&link_type=abstract

Publications of the Astronomical Society of the Pacific, Volume 121, issue 878, pp.350-358

Astronomy and Astrophysics

Astronomy

9

Stars

Scientific paper

Infrared spectra are presented for a magnitude-limited (ρ Oph core),
suggesting either a more advanced evolutionary state or a difference in
the intrinsic stellar birthline for very young clusters. We discuss the
implications of our results for the shape of the initial mass function
of the embedded young cluster and the star-forming history of the cloud.

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