N. Castro, M. Roth, P. Weilbacher, G. Micheva, A. Monreal-Ibero, A. Kelz, S. Kamann, M. Maseda, M. Wendt, T. M. C. L. F. A. Potsdam, Instituto de Astrof'isica de Canarias, U. L. Laguna, Liverpool John Moores University, Leiden University, U. Potsdam
{"title":"用MUSE-NFM绘制狼蛛星云中最年轻和最大质量的恒星","authors":"N. Castro, M. Roth, P. Weilbacher, G. Micheva, A. Monreal-Ibero, A. Kelz, S. Kamann, M. Maseda, M. Wendt, T. M. C. L. F. A. Potsdam, Instituto de Astrof'isica de Canarias, U. L. Laguna, Liverpool John Moores University, Leiden University, U. Potsdam","doi":"10.18727/0722-6691/5223","DOIUrl":null,"url":null,"abstract":"The evolution of the most massive stars is a puzzle with many missing pieces. Statistical analyses are the key to provide anchors to calibrate theory, however performing these studies is an arduous job. The state-of-the-art integral field spectrograph MUSE has stirred up stellar astrophysicists who are excited about the capability to take spectra of up to a thousand stars in a single exposure. The excitement was even higher with the commissioning of the MUSE narrow-field-mode (NFM) that has demonstrated angular resolutions akin to the Hubble Space Telescope. We present the first mapping of the dense stellar core R136 in the Tarantula nebula based on a MUSE-NFM mosaic. We aim to deliver the first homogeneous analysis of the most massive stars in the local Universe and to explore the impact of these peculiar objects to the interstellar medium.","PeriodicalId":8493,"journal":{"name":"arXiv: Solar and Stellar Astrophysics","volume":null,"pages":null},"PeriodicalIF":0.0000,"publicationDate":"2021-02-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"2","resultStr":"{\"title\":\"Mapping the Youngest and Most Massive Stars in the Tarantula Nebula with MUSE-NFM\",\"authors\":\"N. Castro, M. Roth, P. Weilbacher, G. Micheva, A. Monreal-Ibero, A. Kelz, S. Kamann, M. Maseda, M. Wendt, T. M. C. L. F. A. Potsdam, Instituto de Astrof'isica de Canarias, U. L. Laguna, Liverpool John Moores University, Leiden University, U. Potsdam\",\"doi\":\"10.18727/0722-6691/5223\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"The evolution of the most massive stars is a puzzle with many missing pieces. Statistical analyses are the key to provide anchors to calibrate theory, however performing these studies is an arduous job. The state-of-the-art integral field spectrograph MUSE has stirred up stellar astrophysicists who are excited about the capability to take spectra of up to a thousand stars in a single exposure. The excitement was even higher with the commissioning of the MUSE narrow-field-mode (NFM) that has demonstrated angular resolutions akin to the Hubble Space Telescope. We present the first mapping of the dense stellar core R136 in the Tarantula nebula based on a MUSE-NFM mosaic. We aim to deliver the first homogeneous analysis of the most massive stars in the local Universe and to explore the impact of these peculiar objects to the interstellar medium.\",\"PeriodicalId\":8493,\"journal\":{\"name\":\"arXiv: Solar and Stellar Astrophysics\",\"volume\":null,\"pages\":null},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2021-02-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"2\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"arXiv: Solar and Stellar Astrophysics\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.18727/0722-6691/5223\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv: Solar and Stellar Astrophysics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.18727/0722-6691/5223","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Mapping the Youngest and Most Massive Stars in the Tarantula Nebula with MUSE-NFM
The evolution of the most massive stars is a puzzle with many missing pieces. Statistical analyses are the key to provide anchors to calibrate theory, however performing these studies is an arduous job. The state-of-the-art integral field spectrograph MUSE has stirred up stellar astrophysicists who are excited about the capability to take spectra of up to a thousand stars in a single exposure. The excitement was even higher with the commissioning of the MUSE narrow-field-mode (NFM) that has demonstrated angular resolutions akin to the Hubble Space Telescope. We present the first mapping of the dense stellar core R136 in the Tarantula nebula based on a MUSE-NFM mosaic. We aim to deliver the first homogeneous analysis of the most massive stars in the local Universe and to explore the impact of these peculiar objects to the interstellar medium.
京公网安备 11010802042870号
京ICP备2023020795号-1
分享
求助内容：
应助结果提醒方式：
扫码关注我们
