메뉴 건너뛰기




Volumn 506, Issue 1, 2009, Pages 95-101

The B0.5IVe CoRoT target HD49330∗ I. Photometric analysis from CoRoT data

Author keywords

Stars: early type; Stars: emission line, Be; Stars: individual: HD49330; Stars: oscillations; Stars: rotation

Indexed keywords

CURVE FITTING; LEAST SQUARES APPROXIMATIONS;

EID: 84977566904     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200911928     Document Type: Article
Times cited : (124)

References (17)
  • 11
    • 0009777581 scopus 로고    scopus 로고
    • In IAU coll
    • 175 The Be Phenomenon in Early-Type Stars, ed. M. A. Smith, H. F. Henrichs, & J. Fabregat
    • Hubert, A. M., Floquet, M., & Zorec, J. 2000, in IAU Coll., 175, The Be Phenomenon in Early-Type Stars, ed. M. A. Smith, H. F. Henrichs, & J. Fabregat, ASP Conf. Ser., 214, 348
    • (2000) ASP Conf. Ser. , vol.214 , pp. 348
    • Hubert, A.M.1    Floquet, M.2    Zorec, J.3
  • 17
    • 49749084520 scopus 로고    scopus 로고
    • corrected in [arXiv:astro-ph/0703354]
    • Samadi, R., Fialho, F., Costa, J. E. S., et al. 2006, ESA SP 1306, 317, corrected in [arXiv:astro-ph/0703354]
    • (2006) ESA SP , vol.1306 , pp. 317
    • Samadi, R.1    Fialho, F.2    Costa, J.E.S.3


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.