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Volumn 123, Issue 5 1757, 2002, Pages 2689-2702

21 Centimeter H I line observations of the Cygnus Loop

Author keywords

ISM: H I; Supernova remnants

Indexed keywords


EID: 0042149435     PISSN: 00046256     EISSN: None     Source Type: Journal    
DOI: 10.1086/339703     Document Type: Article
Times cited : (19)

References (19)
  • 1
    • 0002062989 scopus 로고    scopus 로고
    • Röntgenstrahlungfrom the Universe, ed. H. Zim-merman, J. Trumper, & H. Yorke (Garching: MPE extraterr. Phys.)
    • Aschenbach, B. 1996, in Röntgenstrahlungfrom the Universe, ed. H. Zim-merman, J. Trumper, & H. Yorke (MPE Rep. 263) (Garching: MPE extraterr. Phys.), 213
    • (1996) MPE Rep. , vol.263 , pp. 213
    • Aschenbach, B.1
  • 5
    • 0009718825 scopus 로고
    • DeNoyer, L. 1975, ApJ, 196, 479
    • (1975) ApJ , vol.196 , pp. 479
    • DeNoyer, L.1
  • 10
    • 0141431792 scopus 로고    scopus 로고
    • Seeing Through the Dust: The Detection of H I and the Exploration of the ISM in Galaxies (San Francisco: ASP), in press
    • Leahy, D. 2002, in ASP Conf. Ser., Seeing Through the Dust: The Detection of H I and the Exploration of the ISM in Galaxies (San Francisco: ASP), in press
    • (2002) ASP Conf. Ser.
    • Leahy, D.1
  • 11
    • 0141654810 scopus 로고    scopus 로고
    • Röntgenstrahlung from the Universe, ed. H. Zimmerman, J. Trumper, & H. Yorke (Garching: MPE extraterr. Phys.)
    • Leahy, D., & Aschenbach, B. 1996, in Röntgenstrahlung from the Universe, ed. H. Zimmerman, J. Trumper, & H. Yorke (MPE Rep. 263) (Garching: MPE extraterr. Phys.), 261
    • (1996) MPE Rep. , vol.263 , pp. 261
    • Leahy, D.1    Aschenbach, B.2
  • 14
    • 0141431790 scopus 로고    scopus 로고
    • Röntgenstrahlung from the Universe, ed. H. Zimmerman, J. Trumper, & H. Yorke (Garching: MPE extraterr. Phys.)
    • Levenson, N., et al. 1996, in Röntgenstrahlung from the Universe, ed. H. Zimmerman, J. Trumper, & H. Yorke (MPE Rep. 263) (Garching: MPE extraterr. Phys.), 263
    • (1996) MPE Rep. , vol.263 , pp. 263
    • Levenson, N.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.