메뉴 건너뛰기




Volumn 437, Issue 3, 2005, Pages 1017-1021

RR Lyrae variables in Galactic globular clusters: V. The case of M 3 pulsators

Author keywords

Instabilities; Stars: evolution; Stars: Hertzsprung Russell (HR) and C M diagrams; Stars: interiors; Stars: low mass, brown dwarfs; Stars: oscillations

Indexed keywords

ASTROPHYSICS; CALIBRATION; NUCLEAR PHYSICS; OSCILLATIONS; PROBABILITY; RANDOM PROCESSES;

EID: 21844463057     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20042306     Document Type: Article
Times cited : (27)

References (22)
  • 8
    • 1642311983 scopus 로고    scopus 로고
    • Catelan, M. 2004, ApJ, 600, 409
    • (2004) ApJ , vol.600 , pp. 409
    • Catelan, M.1
  • 13
    • 4243345692 scopus 로고
    • Dorman, B. 1992, ApJS, 81, 221
    • (1992) ApJS , vol.81 , pp. 221
    • Dorman, B.1
  • 15
  • 20
    • 0009040821 scopus 로고
    • The use of pulsating stars in fundamental problems of astronomy
    • Cambridge and New York: Cambridge University Press
    • Rood, R. T., & Crocker, D. A. 1989, The Use of Pulsating Stars in Fundamental Problems of Astronomy (Cambridge and New York: Cambridge University Press), IAU Coll., 111, 103
    • (1989) IAU Coll. , vol.111 , pp. 103
    • Rood, R.T.1    Crocker, D.A.2


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.