A DOUBLE CLUSTER AT THE CORE OF 30 DORADUS

被引：69

作者：

Sabbi, E. ^{[1
]}

Lennon, D. J. ^{[2
]}

Gieles, M. ^{[3
]}

de Mink, S. E. ^{[1
,4
]}

Walborn, N. R. ^{[1
]}

Anderson, J. ^{[1
]}

Bellini, A. ^{[1
]}

Panagia, N. ^{[1
]}

van der Marel, R. ^{[1
]}

Maiz Apellaniz, J. ^{[5
]}

机构：

[1] Space Telescope Sci Inst, Baltimore, MD 21218 USA

[2] ESA STScI, Baltimore, MD 21218 USA

[3] Univ Cambridge, Inst Astron, Cambridge CB3 0HA, England

[4] Johns Hopkins Univ, Baltimore, MD 21218 USA

[5] CSIC, Inst Astrofis Andalucia, E-18008 Granada, Spain

来源：

ASTROPHYSICAL JOURNAL LETTERS | 2012年 / 754卷 / 02期

关键词：

galaxies: star clusters: individual (30 Doradus); galaxies: star formation; Magellanic Clouds; LARGE-MAGELLANIC-CLOUD; INITIAL MASS FUNCTION; STAR-FORMATION; SPECTRAL CLASSIFICATION; STELLAR POPULATIONS; STARBURST CLUSTER; MOLECULAR CLOUDS; IONIZING CLUSTER; OB ASSOCIATIONS; SKY SURVEY;

D O I：

10.1088/2041-8205/754/2/L37

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Based on an analysis of data obtained with the Wide Field Camera 3 on the Hubble Space Telescope we report the identification of two distinct stellar populations in the core of the giant H II region 30 Doradus in the Large Magellanic Cloud. The most compact and richest component coincides with the center of R136 and is similar to 1 Myr younger than a second more diffuse clump, located similar to 5.4 pc toward the northeast. We note that published spectral types of massive stars in these two clumps lend support to the proposed age difference. The morphology and age difference between the two sub-clusters suggests that an ongoing merger may be occurring within the core of 30 Doradus. This finding is consistent with the predictions of models of hierarchical fragmentation of turbulent giant molecular clouds, according to which star clusters would be the final products of merging smaller sub-structures.

引用

页数：6

共 42 条

[1] THE LOW-MASS INITIAL MASS FUNCTION IN THE 30 DORADUS STARBURST CLUSTER [J].