Matches in SemOpenAlex for { <https://semopenalex.org/work/W4317941650> ?p ?o ?g. }
Showing items 1 to 53 of
53
with 100 items per page.
- W4317941650 abstract "From TESS photometry, 493 mid- to late-B stars with high frequencies (Maia variables) have been identified. The distribution of projected rotational velocities shows that the rotation rates of Maia variables are no different from those of SPB stars. Moreover, many Maia stars pulsate with frequencies exceeding 60 c/d. Rapid rotation is ruled out as a possible factor in understanding the Maia variables. There is clearly a serious problem with current pulsational models. Not only are the models unable to account for the Maia stars, but they also fail to account for the fact that SPB and gamma Dor variables form one continuous instability strip from the cool end of the delta Sct region to the hot end of the beta Cep instability strip. Likewise, there is continuity between the distributions of delta Sct, Maia, and beta Cep variables. In fact, Maia stars seem to be an extension of delta Sct stars to the mid-B type. These observations suggest an interplay between multiple driving mechanisms rather than separate dominant mechanisms for each variability group." @default.
- W4317941650 created "2023-01-25" @default.
- W4317941650 creator A5012327990 @default.
- W4317941650 date "2023-01-23" @default.
- W4317941650 modified "2023-09-28" @default.
- W4317941650 title "Maia variables and other anomalies among pulsating stars" @default.
- W4317941650 doi "https://doi.org/10.48550/arxiv.2301.09280" @default.
- W4317941650 hasPublicationYear "2023" @default.
- W4317941650 type Work @default.
- W4317941650 citedByCount "0" @default.
- W4317941650 crossrefType "posted-content" @default.
- W4317941650 hasAuthorship W4317941650A5012327990 @default.
- W4317941650 hasBestOaLocation W43179416501 @default.
- W4317941650 hasConcept C121332964 @default.
- W4317941650 hasConcept C150739758 @default.
- W4317941650 hasConcept C150846664 @default.
- W4317941650 hasConcept C17352008 @default.
- W4317941650 hasConcept C204843146 @default.
- W4317941650 hasConcept C207821765 @default.
- W4317941650 hasConcept C2524010 @default.
- W4317941650 hasConcept C33923547 @default.
- W4317941650 hasConcept C44870925 @default.
- W4317941650 hasConcept C57879066 @default.
- W4317941650 hasConcept C68271606 @default.
- W4317941650 hasConcept C74050887 @default.
- W4317941650 hasConceptScore W4317941650C121332964 @default.
- W4317941650 hasConceptScore W4317941650C150739758 @default.
- W4317941650 hasConceptScore W4317941650C150846664 @default.
- W4317941650 hasConceptScore W4317941650C17352008 @default.
- W4317941650 hasConceptScore W4317941650C204843146 @default.
- W4317941650 hasConceptScore W4317941650C207821765 @default.
- W4317941650 hasConceptScore W4317941650C2524010 @default.
- W4317941650 hasConceptScore W4317941650C33923547 @default.
- W4317941650 hasConceptScore W4317941650C44870925 @default.
- W4317941650 hasConceptScore W4317941650C57879066 @default.
- W4317941650 hasConceptScore W4317941650C68271606 @default.
- W4317941650 hasConceptScore W4317941650C74050887 @default.
- W4317941650 hasLocation W43179416501 @default.
- W4317941650 hasOpenAccess W4317941650 @default.
- W4317941650 hasPrimaryLocation W43179416501 @default.
- W4317941650 hasRelatedWork W2066113624 @default.
- W4317941650 hasRelatedWork W2145785818 @default.
- W4317941650 hasRelatedWork W2152935934 @default.
- W4317941650 hasRelatedWork W2685727029 @default.
- W4317941650 hasRelatedWork W2973213298 @default.
- W4317941650 hasRelatedWork W3004319856 @default.
- W4317941650 hasRelatedWork W3012427144 @default.
- W4317941650 hasRelatedWork W4300600455 @default.
- W4317941650 hasRelatedWork W69807739 @default.
- W4317941650 hasRelatedWork W89915948 @default.
- W4317941650 isParatext "false" @default.
- W4317941650 isRetracted "false" @default.
- W4317941650 workType "article" @default.