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2002AJ....123.2590L - Astron. J., 123, 2590-2596 (2002/May-0)
Strong emission-line stars identified toward the Rosette nebula.
LI J.Z., WU C.H., CHEN W.P., RECTOR T., CHU Y.H. and IP W.-H.
Abstract (from CDS):
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.
Abstract Copyright: ∼
Journal keyword(s): Stars: Emission-Line, Be - Stars: Pre-Main-Sequence - X-Rays
CDS comments: Table 1: EM* poss. opt. counterpart 'NN' or 'NNA' of 1RXP sources, from a list of Li J.Z.+ in preparation, not published in 2007, objects are not in SIMBAD.
Simbad objects: 8
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