Strong emission-line stars identified toward the Rosette Nebula

被引：10

作者：

Li, JZ ^{[1
]}

Wu, CH

Chen, WP

Rector, T

Chu, YH

Ip, WH

机构：

[1] Natl Cent Univ, Inst Astron, Chungli 32054, Taiwan

[2] Chinese Acad Sci, Natl Astron Observ, Beijing Astron Observ, Beijing 100012, Peoples R China

[3] Natl Opt Astron Observ, Tucson, AZ 85719 USA

[4] Univ Illinois, Dept Astron, Urbana, IL 61801 USA

来源：

ASTRONOMICAL JOURNAL | 2002年 / 123卷 / 05期

关键词：

stars; emission-line; Be; stars : pre-main-sequence; X-rays;

D O I：

10.1086/339971

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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 similar to1.5 kpc.

引用

页码：2590 / 2596

页数：7

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