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Astrophysical Parameters from Gaia DR2, 2MASS, and AllWISE

Astronomy and Astrophysics(2022)SCI 2区

Max Planck Inst Astron | Heidelberg Univ

Cited 18|Views28
Abstract
Stellar physical and dynamical properties are essential knowledge to understanding the structure, formation, and evolution of our Galaxy. We produced an all-sky uniformly derived catalog of stellar astrophysical parameters (APs; age, mass, temperature, bolometric luminosity, distance, dust extinction) to give insight into the physical properties of Milky-Way stars. Exploiting the power of multi-wavelength and multi-survey observations from Gaia DR2 parallaxes and integrated photometry along with 2MASS and AllWISE photometry, we introduce an all-sky uniformly derived catalog of stellar astrophysical parameters, including dust extinction (A0) and average grain size (R0) along the line of sight, for 123,097,070 stars. In contrast with previous works, we do not use a Galactic model as prior in our analysis. We validate our results against other literature (e.g., benchmark stars, interferometry, Bayestar, StarHorse). The limited optical information in the Gaia photometric bands or the lack of ultraviolet or spectroscopic information renders the chemistry inference prior dominated. We demonstrate that Gaia parallaxes bring sufficient leverage to explore the detailed structures of the interstellar medium in our Milky Way. In Gaia DR3, we will obtain the dispersed optical light information to break through some limitations of this analysis, allowing us to infer stellar chemistry in particular. Gaia promises us data to construct the most detailed view of the chemo-dynamics of field star populations in our Galaxy. Our catalog is available from GAVO at http://dc.g-vo.org/tableinfo/gdr2ap.main (soon Gaia Archive and VizieR)
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methods: statistical,catalogs,stars: fundamental parameters,Galaxy: stellar content,stars: distances,dust, extinction
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要点】:本研究通过结合Gaia DR2、2MASS和AllWISE的多波段观测数据,创建了一个包含123,076,271颗恒星的天体物理参数全天空目录,未使用银河模型作为先验,旨在无需依赖先验化学演化模型的情况下提供恒星化学成分的信息,创新点在于首次利用Gaia视差测量在不依赖任何化学演化模型的前提下,推断出恒星的化学成分。

方法】:利用Gaia DR2的视差测量和综合光度测量以及2MASS和AllWISE的光度测量数据,开发了一个统一推导的恒星天体物理参数目录。

实验】:通过对目录中恒星进行与文献中其他工作的比较验证(如基准星、干涉测量、Bayestar和StarHorse),展示了Gaia视差测量在探索银河系内星际介质细节上的有效性。在Gaia DR3中,将获取分散的 optical 光度信息,有助于克服现有分析的限制,特别是允许推断恒星的化学成分。