Gas and Dust Structures of the Protoplanetary Disk around HD 142527

被引:0
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作者
Momose, Munetake [1 ]
Muto, Takayuki [2 ]
Hanawa, Tomoyuki [3 ]
Fukagawa, Misato [4 ]
Tsukagoshi, Takashi [1 ]
Saigo, Kazuya [5 ]
Kataoka, Akimasa [6 ]
Nomura, Hideko [6 ]
Takeuchi, Taku [6 ]
Akiyama, Eiji [5 ]
Ohashi, Nagayoshi [7 ]
Fujiwara, Hideaki [7 ]
Shibai, Hiroshi [4 ]
Kitamura, Yoshimi [8 ]
Inutsuka, Shu-ichiro [9 ]
Kobayashi, Hiroshi [9 ]
Honda, Mitsuhiko [10 ]
Aso, Yusuke [11 ]
Takahashil, Sanemichi Z. [12 ]
机构
[1] Ibaraki Univ, Mito, Ibaraki, Japan
[2] Kogakuin Univ, Shinjuku Ku, Tokyo, Japan
[3] Chiba Univ, Ihage Ku, Chiba, Japan
[4] Osaka Univ, Toyonaka, Osaka 560, Japan
[5] Natl Inst Nat Sci, Natl Astron Observ Japan, Mitaka, Tokyo, Japan
[6] Tokyo Inst Technol, Meguro Ku, Tokyo 152, Japan
[7] Subaru Telescope, Hilo, HI 96720 USA
[8] Japan Aerosp Explorat Agcy, Inst Space & Astronaut Sci, Sagamihara, Kanagawa 2298510, Japan
[9] Nagoya Univ, Nagoya, Aichi 4648601, Japan
[10] Kanagawa Univ, Hiratsuka, Kanagawa, Japan
[11] Univ Tokyo, Bunkyo Ku, Tokyo 113, Japan
[12] Kyoto Univ, Sakyo Ku, Kyoto, Japan
关键词
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中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
HD142527 is a Herbig Fe star accompanied by a disk with ring-like structure. We derive the distributions of dust and gas separately by model fitting and discuss the spatial variation of gas-to-dust mass ratio in the disk. The radial distribution of dust is well approximated by a Gaussian function, while the gas is roughly followed by a power-law distribution between 110 and 400 AU in radius, which is significantly more extended than dust. G/d may reach the order of unity at the northern peak.
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页码:277 / 278
页数:2
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