Strong Emission-Line Stars Identified toward the Rosette Nebula

Details Strong Emission-Line Stars Identified toward the Rosette Nebula Strong Emission-Line Stars Identified toward the Rosette Nebula

May 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aj....123.2590l&link_type=abstract

The Astronomical Journal, Volume 123, Issue 5, pp. 2590-2596.

Astronomy and Astrophysics

Astronomy

10

Stars: Emission-Line, Be, Stars: Pre-Main-Sequence, X-Rays

Scientific paper

Several strong emission-line stars were found in the optical identification of the ROSAT PSPC sources in the Rosette Nebula. These possible X-ray emitters were classified from the low-resolution spectra obtained as Herbig Ae/Be type stars or probable weak-line T Tauri stars. A classical Be star was also identified around one of the X-ray sources studied. Our study supports the conjecture that ROSAT X-ray observations could trace low- and intermediate-mass star formation to a distance of ~1.5 kpc.

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