H 2 Emission Nebulosity Associated with KH 15D | Zendy

A. T. Tokunaga | Zendy; S. E. Dahm | Zendy; W. Gssler | Zendy; Yutaka Hayano | Zendy; Masahiko Hayashi | Zendy; Masanori Iye | Zendy; Tomio Kanzawa | Zendy; Naoto Kobayashi | Zendy; Yukiko Kamata | Zendy; Yosuke Minowa | Zendy; Ko Nedachi | Zendy; Shin Oya | Zendy; TaeSoo Pyo | Zendy; David Saint-Jacques | Zendy; Hiroshi Terada | Zendy; Hideki Takami | Zendy; Naruhisa Takato | Zendy

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H ₂ Emission Nebulosity Associated with KH 15D

Author(s) -

A. T. Tokunaga,

S. E. Dahm,

W. Gssler,

Yutaka Hayano,

Masahiko Hayashi,

Masanori Iye,

Tomio Kanzawa,

Naoto Kobayashi,

Yukiko Kamata,

Yosuke Minowa,

Ko Nedachi,

Shin Oya,

TaeSoo Pyo,

David Saint-Jacques,

Hiroshi Terada,

Hideki Takami,

Naruhisa Takato

Publication year - 2004

Publication title -

the astrophysical journal

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 2.376

H-Index - 489

eISSN - 1538-4357

pISSN - 0004-637X

DOI - 10.1086/382701

Subject(s) - protein filament , subaru telescope , outflow , physics , astrophysics , astronomy , chemistry , meteorology , spectrograph , spectral line , biochemistry

An H$_2$ emission filament is found in close proximity to the unique objectKH 15D using the adaptive optics system of the Subaru Telescope. The morphologyof the filament, the presence of spectroscopic outflow signatures observed byHamilton et al., and the detection of extended H$_2$ emission from KH 15D byDeming, Charbonneau, & Harrington suggest that this filament arises fromshocked H$_2$ in an outflow. The filament extends about 15" to the north of KH15D.Comment: 11 pages, 3 figures, 1 table. Astrophysical Journal Letters, in pres

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