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Volumn 433, Issue 2, 2005, Pages 579-582

The identification of PM 1-322 as a new young high-density planetary nebulae

Author keywords

Planetary nebulae: individual: PM 1 322

Indexed keywords

ASTROPHYSICS; CARRIER CONCENTRATION; ELECTRON TRANSITIONS; GALAXIES; IMAGING SYSTEMS; LIGHT ABSORPTION; LIGHT EMISSION; SPECTROPHOTOMETRY;

EID: 16644371658     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20042218     Document Type: Review
Times cited : (14)

References (24)
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    • 33746980755 scopus 로고
    • Pereira, C. B. 1995, A&AS, 111, 471
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    • From Miras to planetary-nebulae: Which path for stellar evolution? (Montpellier: Editions Frontières)
    • Pottasch, S. R., Ratag, M. A., & Oiling, R. 1990, in From Miras to planetary-nebulae: Which path for stellar evolution? Proc. International Coll. (Montpellier: Editions Frontières), 381
    • (1990) Proc. International Coll. , pp. 381
    • Pottasch, S.R.1    Ratag, M.A.2    Oiling, R.3
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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.