GALExtin: A VO-Service for Estimating Galactic Interstellar Extinction

机译：GALExtin：估计银河星际灭绝的VO服务

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The distribution of interstellar matter is a fundamental aspect of the structure of our Galaxy. Its knowledge is critical for determining distances and color corrections, for star counts and brightness models of the Galaxy, and also for extinction corrections of spectra, among other applications. In this context, we are developing a VO -Service called GALExtin that provides interstellar extinction estimates for any direction in the sky using available 2D maps, 3D models, catalogs with extinction and diffuse emission measurements. The service is naturally useful for estimating interstellar extinction toward star clusters.

机译：星际物质的分布是我们银河结构的基本方面。它的知识对于确定距离和色彩校正，对于星系的星数和亮度模型以及光谱的消光校正等至关重要。在这种情况下，我们正在开发一种名为GALExtin的VO服务，该服务使用可用的2D地图，3D模型，具有消光和散射发射测量值的目录为天空中的任何方向提供星际消光估计。该服务自然可用于估算星际对星团的灭绝。

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《Star clusters in the era of large surveys》|2010年|p.93-95|共3页
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Eduardo Amores; Andre Moitinho; Vladan Arsenijevic; Laerte Sodre;
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SIM, U. of Lisbon, Campo Grande, Ediffcio C8, Piso 5, 1749-016 Lisboa, Portugal;

SIM, U. of Lisbon, Campo Grande, Ediffcio C8, Piso 5, 1749-016 Lisboa, Portugal;

SIM, U. of Lisbon, Campo Grande, Ediffcio C8, Piso 5, 1749-016 Lisboa, Portugal;

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正文语种 eng
中图分类天文学;
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1. Interstellar extinction law toward the Galactic center. IV. J, H, and K-s bands from VVV red clump stars [J] . Nagatomo Schun, Nagata Tetsuya, Nishiyama Shogo PASJ: Publications of the Astronomical Society of Japan . 2019,第5期

机译：星际灭绝法对银河中心。 IV。来自VVV红丛星星的J，H和K-S频段
2. A measurement of interstellar polarization and an estimation of Galactic extinction for the direction of the X-ray black hole binary V404 Cygni [J] . Ryosuke Itoh, Yasuyuki T. Tanaka, Koji S. Kawabata, PASJ: Publications of the Astronomical Society of Japan . 2017,第2期

机译：星际极化的测量和银河沿X射线黑洞二进制V404 Cygni方向的消光估计
3. Three-dimensional interstellar extinction map toward the Galactic bulge [J] . B. Q. Chen, M. Schultheis, B. W. Jiang, Astronomy and astrophysics . 2013,第19期

机译：朝向银河凸起的三维星际灭绝图
4. Visual Interstellar Extinction in the Galactic Disk [C] . J. GUARINOS International Workshop on the "Evolution of Interstellar Matter and Dynamics of Galaxies" . 1992

机译：在银河磁盘中的视觉星际灭绝
5. Unveiling the Diffuse, Neutral Interstellar Medium: Absorption Spectroscopy of Galactic Hydrogen [D] . Murray, Claire Elizabeth. 2017

机译：揭示漫反射，中性间隙介质：银河系氢的吸收光谱
6. Interstellar Chemistry Special Feature: The galactic cosmic ray ionization rate [O] . A. Dalgarno 2006

机译：星际化学的特长：银河系宇宙射线的电离率
7. Toward understanding the 3.4 μm and 9.7 μm extinction feature variations from the local diffuse interstellar medium to the Galactic center [O] . Jian Gao, B. W. Jiang, Aigen Li 2010

机译：为了理解从局部弥散星际介质到银河系中心的3.4μm和9.7μm消光特征的变化
8. Interstellar Extinction in the Vicinity of the Galactic Center [R] . Cotera, Angela S., Simpson, Janet P., Erickson, Edwin F., 2000

机译：银河系中心附近的星际灭绝

GALExtin: A VO-Service for Estimating Galactic Interstellar Extinction

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