Matches in SemOpenAlex for { <https://semopenalex.org/work/W19279526> ?p ?o ?g. }
Showing items 1 to 51 of
51
with 100 items per page.
- W19279526 abstract "The observed central velocity dispersion of a stellar system is dependent on the mass distribution and the velocity distribution function. For the past several years a program has been undertaken to determine central velocity dispersions of LMC and SMC clusters for comparison with galactic clusters. The mass-to-light ratio (M/L) estimates so obtained should be considerably more accurate than those obtained by tidal arguments (Chun 1978, Elson & Freeman 1985). Accurate radial velocities (mean error = 1.3 km s −1 ) have been obtained for a sample of K-type giants with the CTIO 4m telescope and échelle spectrograph with CCD detector. All of the stars observed were within two core radii of the cluster centre. Multiple observations at several epochs (1984 and 1989) were used to determine the velocity errors. The central M/L in solar units has been estimated from single component isotropic King models (King 1966), with the assumption that the distribution of mass follows that of the light. Observed values for the total integrated light and core radius were taken from the literature (in particular, from Chun 1978, van den Bergh 1981, Mateo 1987)." @default.
- W19279526 created "2016-06-24" @default.
- W19279526 creator A5015336821 @default.
- W19279526 date "1991-01-01" @default.
- W19279526 modified "2023-10-18" @default.
- W19279526 title "Mass-to-light ratio of intermediate and old clusters in the Magellanic Clouds" @default.
- W19279526 cites W1980769538 @default.
- W19279526 cites W2034516476 @default.
- W19279526 cites W2041508062 @default.
- W19279526 cites W2049578501 @default.
- W19279526 doi "https://doi.org/10.1017/s0074180900200417" @default.
- W19279526 hasPublicationYear "1991" @default.
- W19279526 type Work @default.
- W19279526 sameAs 19279526 @default.
- W19279526 citedByCount "0" @default.
- W19279526 crossrefType "journal-article" @default.
- W19279526 hasAuthorship W19279526A5015336821 @default.
- W19279526 hasBestOaLocation W192795261 @default.
- W19279526 hasConcept C121332964 @default.
- W19279526 hasConcept C1276947 @default.
- W19279526 hasConcept C44870925 @default.
- W19279526 hasConceptScore W19279526C121332964 @default.
- W19279526 hasConceptScore W19279526C1276947 @default.
- W19279526 hasConceptScore W19279526C44870925 @default.
- W19279526 hasLocation W192795261 @default.
- W19279526 hasOpenAccess W19279526 @default.
- W19279526 hasPrimaryLocation W192795261 @default.
- W19279526 hasRelatedWork W1619921699 @default.
- W19279526 hasRelatedWork W2129949945 @default.
- W19279526 hasRelatedWork W2503644871 @default.
- W19279526 hasRelatedWork W2616088509 @default.
- W19279526 hasRelatedWork W2993526658 @default.
- W19279526 hasRelatedWork W2995812673 @default.
- W19279526 hasRelatedWork W3004211482 @default.
- W19279526 hasRelatedWork W3005699255 @default.
- W19279526 hasRelatedWork W3017205076 @default.
- W19279526 hasRelatedWork W3017867378 @default.
- W19279526 hasRelatedWork W3025956143 @default.
- W19279526 hasRelatedWork W3032117551 @default.
- W19279526 hasRelatedWork W3042280958 @default.
- W19279526 hasRelatedWork W3087574907 @default.
- W19279526 hasRelatedWork W3130466598 @default.
- W19279526 hasRelatedWork W3134859731 @default.
- W19279526 hasRelatedWork W3164538474 @default.
- W19279526 hasRelatedWork W3172013547 @default.
- W19279526 hasRelatedWork W3174063461 @default.
- W19279526 hasRelatedWork W3116062712 @default.
- W19279526 isParatext "false" @default.
- W19279526 isRetracted "false" @default.
- W19279526 magId "19279526" @default.
- W19279526 workType "article" @default.