YOUNG STARS IN THE LMC PERIPHERY

被引：0

作者：

Bidin, C. Moni ^{[1
]}

Casetti-Dinescu, D. I. ^{[2
]}

Girard, T. M. ^{[3
]}

Zhang, L. ^{[4
,5
]}

Mendez, R. A. ^{[6
]}

Vieira, K. ^{[7
]}

Korchagin, V. I. ^{[8
]}

van Altena, W. F. ^{[9
]}

机构：

[1] Univ Catolica Norte, Inst Astron, Ave Angamos 0610, Antofagasta, Chile

[2] Southern Connecticut State Univ, Dept Phys, 501 Crescent St, New Haven, CT 06515 USA

[3] 14 Dunn Rd, Hamden, CT 06518 USA

[4] CAS South Amer Ctr Astron, Camino El Observ 1515, Santiago, Chile

[5] Chinese Acad Sci, Natl Astron Observ, Key Lab Opt Astron, 20A Datun Rd, Beijing 100012, Peoples R China

[6] Univ Chile, Dept Astron, Casilla 36-D, Santiago, Chile

[7] Ctr Invest Astron, Apartado Postal 264, Merida 5101A, Venezuela

[8] Southern Fed Univ, Inst Phys, Stachki St 124, Rostov Na Donu, Russia

[9] Yale Univ, Dept Astron, POB 208101, New Haven, CT 06520 USA

来源：

XV LATIN AMERICAN REGIONAL IAU MEETING, 2016 | 2017年 / 49卷

关键词：

MAGELLANIC CLOUDS;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We report the discovery of six young (10-50 Myr) main-sequence stars projected between 7 degrees and 13 degrees from the center of the Large Magellanic Cloud (LMC). These stars have low to moderate velocity differences with the predictions of a LMC disk model, indicating that they were formed in situ. Our study demonstrates that recent star formation occurred in the far periphery of the LMC, where thus far only old objects were known. The spatial configuration of these newly-forthed stars appears ring-like.

引用

页码：108 / 108

页数：1

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