Adaptive optics spectroscopy of the [Fe II] outflows from HL Tauri and RW Aurigae

Astrophysical Journal

Volumn 649, Issue 2 I, 2006, Pages 836-844

  Pyo, Tae Soo ^a   Hayashi, Masahiko ^a,b   Kobayashi, Naoto ^c   Tokunaga, Alan T ^d   Terada, Hiroshi ^a   Takami, Hideki ^a,b   Takato, Naruhisa ^a,b   Davis, Christoper J ^d   Takami, Michihiro ^a   Hayashi, Saeko S ^a,b   Gässler, Wolfgang ^a,e   Oya, Shin ^a   Hayano, Yutaka ^a   Kamata, Yukiko ^a   Minowa, Yosuke ^c   Iye, Masanori ^a,b   Usuda, Tomonori ^a,b   Nishikawa, Takayuki ^b   Nedachi, Ko ^c  

^a NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^b GRADUATE UNIVERSITY FOR ADVANCED STUDIES   (Japan)

^c UNIVERSITY OF TOKYO   (Japan)

^d UNIVERSITY OF HAWAII   (United States)

^e MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

Author keywords

ISM: Herbig Haro objects; ISM: individual (HLTauri: HH 150, RW Aurigae: HH 229); ISM: jets and outflows; Stars: formation; Stars: pre main sequence; Techniques: high angular resolution

Indexed keywords

EID: 34250742270     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/506929     Document Type: Article

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