KMS Of Academy of mathematics and systems sciences, CAS
The Young Stars in the Galactic Center | |
von Fellenberg, Sebastiano D.1,2; Gillessen, Stefan2; Stadler, Julia3; Bauboeck, Michi4; Genzel, Reinhard2,5,6; de Zeeuw, Tim2,7; Pfuhl, Oliver8; Seoane, Pau Amaro2,9,10,11; Drescher, Antonia2; Eisenhauer, Frank2; Habibi, Maryam2; Ott, Thomas2; Widmann, Felix2; Young, Alice2 | |
2022-06-01 | |
发表期刊 | ASTROPHYSICAL JOURNAL LETTERS |
ISSN | 2041-8205 |
卷号 | 932期号:1页码:29 |
摘要 | We present a large similar to 30 '' x 30 '' spectroscopic survey of the Galactic Center using the SINFONI IFU at the VLT. Combining observations of the last two decades we compile spectra of over 2800 stars. Using the Bracket-gamma absorption lines, we identify 195 young stars, extending the list of known young stars by 79. In order to explore the angular momentum distribution of the young stars, we introduce an isotropic cluster prior. This prior reproduces an isotropic cluster in a mathematically exact way, which we test through numerical simulations. We calculate the posterior angular momentum space as a function of projected separation from Sgr A*. We find that the observed young star distribution is substantially different from an isotropic cluster. We identify the previously reported feature of the clockwise disk and find that its angular momentum changes as a function of separation from the black hole and thus confirm a warp of the clockwise disk (p similar to 99.2%). At large separations, we discover three prominent overdensities of the angular momentum. One overdensity has been reported previously, the counterclockwise disk. The other two are new. Determining the likely members of these structures, we find that as many as 75% of stars can be associated with one of these features. Stars belonging to the warped clockwise disk show a top-heavy K-band luminosity function, while stars belonging to the larger separation features do not. Our observations are in good agreement with the predictions of simulations of in situ star formation and argue for the common formation of these structures. |
DOI | 10.3847/2041-8213/ac68ef |
收录类别 | SCI |
语种 | 英语 |
资助项目 | Max Planck International Research School |
WOS研究方向 | Astronomy & Astrophysics |
WOS类目 | Astronomy & Astrophysics |
WOS记录号 | WOS:000809245700001 |
出版者 | IOP Publishing Ltd |
引用统计 | |
文献类型 | 期刊论文 |
条目标识符 | http://ir.amss.ac.cn/handle/2S8OKBNM/61491 |
专题 | 中国科学院数学与系统科学研究院 |
通讯作者 | von Fellenberg, Sebastiano D. |
作者单位 | 1.Max Planck Inst Radio Astron, Hugel 69, D-53121 Bonn, Germany 2.Max Planck Inst Extraterr Phys, Giessenbachstr 1, D-85748 Garching, Germany 3.Max Planck Inst Astrophys, Karl Schwarzschild Str 1, D-85748 Garching, Germany 4.Univ Illinois, 1002 W Green St, Urbana, IL 61801 USA 5.Univ Calif Berkeley, Dept Phys, Le Conte Hall, Berkeley, CA 94720 USA 6.Univ Calif Berkeley, Dept Astron, Le Conte Hall, Berkeley, CA 94720 USA 7.Leiden Univ, Sterrewacht Leiden, Postbus 9513, NL-2300 RA Leiden, Netherlands 8.European Southern Observ, Karl Schwarzschild Str 2, D-85748 Garching, Germany 9.Univ Politecn Valencia, Inst Multidisciplinary Math, Valencia, Spain 10.Peking Univ, Kavli Inst Astron & Astrophys, Beijing, Peoples R China 11.Chinese Acad Sci, AMSS, Beijing, Peoples R China |
推荐引用方式 GB/T 7714 | von Fellenberg, Sebastiano D.,Gillessen, Stefan,Stadler, Julia,et al. The Young Stars in the Galactic Center[J]. ASTROPHYSICAL JOURNAL LETTERS,2022,932(1):29. |
APA | von Fellenberg, Sebastiano D..,Gillessen, Stefan.,Stadler, Julia.,Bauboeck, Michi.,Genzel, Reinhard.,...&Young, Alice.(2022).The Young Stars in the Galactic Center.ASTROPHYSICAL JOURNAL LETTERS,932(1),29. |
MLA | von Fellenberg, Sebastiano D.,et al."The Young Stars in the Galactic Center".ASTROPHYSICAL JOURNAL LETTERS 932.1(2022):29. |
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