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Volumn 416, Issue 2, 2004, Pages 713-732

Flares from small to large: X-ray spectroscopy of Proxima Centauri with XMM-Newton

Author keywords

Stars: activity; Stars: coronae; Stars: individual: Proxima Centauri; X rays: stars

Indexed keywords

CARRIER CONCENTRATION; COMPUTER SIMULATION; COOLING; IONIZATION; OSCILLATORS (ELECTRONIC); PLASMAS; SATELLITES; SUN; X RAY SPECTROSCOPY;

EID: 1642364978     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20031471     Document Type: Article
Times cited : (133)

References (86)
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    • Güdel, M. 1997, ApJ, 480, L121
    • (1997) ApJ , vol.480
    • Güdel, M.1
  • 27
    • 85039577159 scopus 로고    scopus 로고
    • Highly Energetic Physical Processes and Mechanisms for Emissions from Astrophysical Plasmas, ed. P. C. H. Martens, S. Tsuruta, & M. A. Weber (San Francisco: ASP)
    • Güdel, M. 2000, in Highly Energetic Physical Processes and Mechanisms for Emissions from Astrophysical Plasmas, ed. P. C. H. Martens, S. Tsuruta, & M. A. Weber (San Francisco: ASP), IAU Symp., 195, 395
    • (2000) IAU Symp. , vol.195 , pp. 395
    • Güdel, M.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.