Abundant circumstellar silica dust and sio gas created by a giant hypervelocity collision in the 12 myr hd172555 system

Astrophysical Journal

Volumn 701, Issue 2, 2009, Pages 2019-2032

  Lisse, C M ^a   Chen, C H ^b   Wyatt, M C ^c   Morlok, A ^d,h   Song, I ^e   Bryden, G ^f   Sheehan, P ^g  

^a JHU/APL   (United States)

^b STScI   (United States)

^c UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^d OPEN UNIVERSITY   (United Kingdom)

^e UNIVERSITY OF GEORGIA   (United States)

^f CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^g UNIVERSITY OF ROCHESTER   (United States)

^h CRPG CNRS   (France)

Author keywords

Astrochemistry; Infrared: stars; Planetary systems: formation; Planetary systems: protoplanetary disks; Radiation mechanisms: thermal; Techniques: spectroscopic

Indexed keywords

EID: 70549102379     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/701/2/2019     Document Type: Article

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