Stellar X-ray sources in the Rosette Nebula

被引：6

作者：

Chen, WP ^{[1
]}

Chiang, PS

Li, JZ

机构：

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

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

来源：

CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS | 2004年 / 4卷 / 02期

关键词：

stars : early-type; stars : pre-main sequence; stars : formation; HII regions;

D O I：

10.1088/1009-9271/4/2/153

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present optical photometric and spectroscopic studies of ROSAT X-ray stellar sources in the Rosette Nebula star-forming region. The brightest Xray sources are either massive stars or active T Tauri stars associated with the open cluster NGC 2244, or are foreground stars. Some of the spectra of the young stars newly identified in the region are presented.

引用

页码：153 / 165

页数：13

共 25 条

[1] Berghofer TW, 1997, ASTRON ASTROPHYS, V322, P167
[2] Optical properties of X-ray selected stars in NGC 2244 in the Rosette Nebula
Berghöfer, TW
Christian, DJ
[J]. ASTRONOMY & ASTROPHYSICS, 2002, 384 (03) : 890 - 898
[3] Chiang PS, 2001, ASTR SOC P, V246, P335
[4] CLAYTON CA, 1995, ASTRON ASTROPHYS, V302, P202
[5] Clayton CA, 1998, ASTRON ASTROPHYS, V334, P264
[6] A search for spectroscopic binaries among Herbig Ae Be stars
Corporon, P
Lagrange, AM
[J]. ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES, 1999, 136 (03): : 429 - 444
[7] COX P, 1990, ASTRON ASTROPHYS, V230, P181
[8] High-energy processes in young stellar objects
Feigelson, ED
Montmerle, T
[J]. ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, 1999, 37 : 363 - 408
[9] Flaccomio E, 2000, ASTRON ASTROPHYS, V355, P651
[10] Gregorio-Hetem J, 1998, ASTRON ASTROPHYS, V331, P193

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