SCOPUS 정보 검색 플랫폼

Monthly Notices of the Royal Astronomical Society

Volumn 299, Issue 4, 1998, Pages 929-941

On the prospect of inferring the halo structure and the masses of dark objects through parallax microlensing

(1) Markovic D a,b

a THEORETICAL ASTROPHYSICS CENTER (Denmark)

b UNIVERSITY OF ILLINOIS AT URBANA CHAMPAIGN (United States)

Author keywords

Dark matter; Galaxy: fundamental parameters; Galaxy: halo; Galaxy: kinematics and dynamics; Gravitational lensing

Indexed keywords

ERRORS; FUNCTIONS; GALAXIES; GRAVITATION; KINEMATICS;

DARK MATTER; GALAXIES: FUNDAMENTAL PARAMETERS; GALAXIES: KINEMATICS AND DYNAMICS; GALAXY:HALO; GRAVITATIONAL LENSING; HALO STRUCTURE; LARGE MAGELLANIC CLOUDS; MASS FUNCTIONS; MICRO-LENSING; POWER-LAW;

GEOMETRICAL OPTICS;

EID: 0009948277 PISSN: 00358711 EISSN: None Source Type: Journal
DOI: 10.1046/j.1365-8711.1998.01627.x Document Type: Article

Times cited : (4)

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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.