Strong emission-line stars identified toward the Rosette Nebula

J. Z. Li; C. H. Wu; W. P. Chen; T. Rector; Y. H. Chu; W. H. Ip

doi:10.1086/339971

Strong emission-line stars identified toward the Rosette Nebula

J. Z. Li, C. H. Wu, W. P. Chen, T. Rector, Y. H. Chu, W. H. Ip

天文研究所

研究成果: 雜誌貢獻 › 期刊論文 › 同行評審

8 引文斯高帕斯（Scopus）

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 ∼1.5 kpc.

原文	???core.languages.en_GB???
頁（從 - 到）	2590-2596
頁數	7
期刊	Astronomical Journal
卷	123
發行號	5 1757
DOIs	https://doi.org/10.1086/339971
出版狀態	已出版 - 5月 2002

存取文件

10.1086/339971

引用此

@article{62326758202d499ca8347d799abd7082,

title = "Strong emission-line stars identified toward the Rosette Nebula",

abstract = "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.",

keywords = "Stars: emission-line, Be, Stars: pre-main-sequence, X-rays",

author = "Li, {J. Z.} and Wu, {C. H.} and Chen, {W. P.} and T. Rector and Chu, {Y. H.} and Ip, {W. H.}",

year = "2002",

month = may,

doi = "10.1086/339971",

language = "???core.languages.en_GB???",

volume = "123",

pages = "2590--2596",

journal = "Astronomical Journal",

issn = "0004-6256",

number = "5 1757",

}

TY - JOUR

T1 - Strong emission-line stars identified toward the Rosette Nebula

AU - Li, J. Z.

AU - Wu, C. H.

AU - Chen, W. P.

AU - Rector, T.

AU - Chu, Y. H.

AU - Ip, W. H.

PY - 2002/5

Y1 - 2002/5

N2 - 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.

AB - 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.

KW - Stars: emission-line, Be

KW - Stars: pre-main-sequence

KW - X-rays

UR - http://www.scopus.com/inward/record.url?scp=0041734386&partnerID=8YFLogxK

U2 - 10.1086/339971

DO - 10.1086/339971

M3 - 期刊論文

AN - SCOPUS:0041734386

SN - 0004-6256

VL - 123

SP - 2590

EP - 2596

JO - Astronomical Journal

JF - Astronomical Journal

IS - 5 1757

ER -

Strong emission-line stars identified toward the Rosette Nebula

摘要

存取文件

指紋

引用此