AKARI results on the Taurus-Auriga star forming region

被引：0

作者：

Zahorecz, Sarolta ^{[1
]}

Toth, L. Viktor ^{[1
]}

Munetaka, Ueno ^{[2
]}

Marton, Gabor ^{[1
]}

Kawamura, Akiko ^{[3
]}

Tamura, Motohide ^{[4
]}

机构：

[1] Eotvos Lorand Univ, Dept Astron, POB 32, H-1518 Budapest, Hungary

[2] Univ Tokyo, Grad Sch Arts & Sci, Dept Earth Sci, Tokyo 1138654, Japan

[3] Nagoya Univ, Grad Sch Sci, Div Particle & Astrophys, Nagoya, Aichi 464, Japan

[4] Natl Astron Observ Japan, Mitaka, Tokyo 1818588, Japan

来源：

5TH WORKSHOP OF YOUNG RESEARCHERS IN ASTRONOMY & ASTROPHYSICS | 2010年 / 218卷

基金：

美国国家科学基金会; 美国国家航空航天局;

关键词：

MAIN-SEQUENCE STARS;

D O I：

10.1088/1742-6596/218/1/012022

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present an analysis of AKARI Far-Infrared Surveyor, Spitzer Space Telescope Infrared Array Camera and Mid-Infrared Photometer for Spitzer data as well as various other photometric data of the Taurus-Auriga region. Our aim was to locate and describe young stellar objects (YSO), and to test the potential of AKARI FIS data in the classification of YSOs. We studied 32 YSOs, 7 of those had not been observed by the SST. We succesfully modeled 21 YSOs with the SED Fitting Tool of Robitaille. We confirmed the previous models in 20 cases, and corrected the physical parameters for 5 YSOs. This research is part of the AKARI Mission Program "Star Formation".

引用

页数：4

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