SUBARU follow-up observation of class 0 sources detected by Chandra X-ray observatory

被引：0

作者：

Tsujimoto, M ^{[1
]}

Koyama, K ^{[1
]}

Goto, M ^{[1
]}

Terada, H ^{[1
]}

Kobayashi, N ^{[1
]}

Tsuboi, Y ^{[1
]}

机构：

[1] Kyoto Univ, Dept Phys, Grad Sch Sci, Sakyo Ku, Kyoto 6068502, Japan

来源：

NEW CENTURY OF X-RAY ASTRONOMY | 2001年 / 251卷

关键词：

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Follow-up observations of the X-ray emitting class 0 candidates were performed in the near infrared hand using the SUBARU telescope. We set the upper limit on the K-band magnitude of these candidates, and found a jet-like feature in H-2 v = 1-0 S(1) band, originating from one of these candidates. These sources, therefore, arc, more likely to be class 0s, and thus are the first discoveries of the X-ray emitting class 0 objects.

引用

页码：282 / 283

页数：2

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