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Volumn 154, Issue 1, 2004, Pages 402-407

Is the Cepheus E outflow driven by a class 0 protostar?

Author keywords

Infrared: stars; ISM: Herbig Haro objects; ISM: individual (Cepheus E); ISM: jets and outflows; ISM: molecules; Stars: formation

Indexed keywords


EID: 5644224696     PISSN: 00670049     EISSN: None     Source Type: Journal    
DOI: 10.1086/423136     Document Type: Article
Times cited : (42)

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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.