메뉴 건너뛰기




Volumn 423, Issue 3, 2004, Pages 1095-1099

Extending the radio spectrum of magnetic chemically peculiar stars to the mm range

Author keywords

Radio continuum: stars; Stars: chemically peculiar; Stars: circumstellar matter; Stars: individual: HD 35298, HD 124224; Stars: magnetic field

Indexed keywords

BANDWIDTH; DATA REDUCTION; ERROR ANALYSIS; INTERFEROMETERS; LIGHT; MAGNETIC FIELDS; MAGNETIC FLUX; MAGNETOSPHERE; RADIO; SYNTHESIS (CHEMICAL);

EID: 4243070831     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20040181     Document Type: Article
Times cited : (13)

References (16)
  • 2
  • 5
    • 4243093269 scopus 로고
    • Evidence for non-radiative activity in hot stars
    • ed. A. B. Underbill, & A. G. Michalitsianos, NASA CP-2358, 2
    • Cassinelli, J. P. 1984, Evidence for non-radiative activity in hot stars, in The Origin of Nonradiative Heating/Momentum in Hot Stars, ed. A. B. Underbill, & A. G. Michalitsianos, NASA CP-2358, 2
    • (1984) The Origin of Nonradiative Heating/Momentum in Hot Stars
    • Cassinelli, J.P.1
  • 12
    • 0011114086 scopus 로고
    • Leone, F. 1991, A&A, 252, 198
    • (1991) A&A , vol.252 , pp. 198
    • Leone, F.1
  • 15
    • 0000464620 scopus 로고
    • Ramaty, R. 1969, ApJ, 158, 753
    • (1969) ApJ , vol.158 , pp. 753
    • Ramaty, R.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.