FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2111418547> ?p ?o ?g. }

• W2111418547 endingPage "1351" @default.
• W2111418547 startingPage "1339" @default.
• W2111418547 abstract "We carried out a multi-colour time-series photometric study of six stars claimed as hybrid p and g mode pulsators in the literature. Gamma Peg was confirmed to show short-period oscillations of the Beta Cep type and simultaneous long-period pulsations typical of Slowly Pulsating B (SPB) stars. From the measured amplitude ratios in the Stromgren uvy passbands, the stronger of the two short period pulsation modes was identified as radial; the second is l=1. Three of the four SPB-type modes are most likely l=1 or 2. Comparison with theoretical model calculations suggests that Gamma Peg is either an 8.5 solar mass radial fundamental mode pulsator or a 9.6 solar mass first radial overtone pulsator. HD 8801 was corroborated as a hybrid Delta Sct Gamma Dor star; four pulsation modes of the Gamma Dor type were detected, and two modes of the Delta Sct type were confirmed. Two pulsational signals between the frequency domains of these two known classes of variables were confirmed and another was newly detected. These are either previously unknown types of pulsation, or do not originate from HD 8801. The O-type star HD 13745 showed small-amplitude slow variability on a time scale of 3.2 days. This object may be related to the suspected new type of supergiant SPB stars, but a rotational origin of its light variations cannot be ruled out at this point. 53 Psc is an SPB star for which two pulsation frequencies were determined and identified with low spherical degree. The behaviour of 53 Ari and Iota Her is consistent with non-variability during our observations, and we could not confirm light variations of the comparison star 34 Psc previously suspected. The use of signal-to-noise criteria in the analysis of data sets with strong aliasing is critically discussed." @default.
• W2111418547 created "2016-06-24" @default.
• W2111418547 creator A5010037298 @default.
• W2111418547 date "2009-09-21" @default.
• W2111418547 modified "2023-09-23" @default.
• W2111418547 title "Confirmation of simultaneous p and g mode excitation in HD 8801 and γ Peg from time-resolved multicolour photometry of six candidate ‘hybrid’ pulsators" @default.
• W2111418547 cites W1493143916 @default.
• W2111418547 cites W1494524745 @default.
• W2111418547 cites W1501612951 @default.
• W2111418547 cites W1661200856 @default.
• W2111418547 cites W1778790332 @default.
• W2111418547 cites W1927717723 @default.
• W2111418547 cites W1960445990 @default.
• W2111418547 cites W1966144665 @default.
• W2111418547 cites W1971993008 @default.
• W2111418547 cites W1977260818 @default.
• W2111418547 cites W1985833364 @default.
• W2111418547 cites W1985836609 @default.
• W2111418547 cites W1988399757 @default.
• W2111418547 cites W1989430366 @default.
• W2111418547 cites W2004261090 @default.
• W2111418547 cites W2004315054 @default.
• W2111418547 cites W2010657815 @default.
• W2111418547 cites W2012853668 @default.
• W2111418547 cites W2023086951 @default.
• W2111418547 cites W2026102027 @default.
• W2111418547 cites W2033784390 @default.
• W2111418547 cites W2034337646 @default.
• W2111418547 cites W2034849524 @default.
• W2111418547 cites W2036847305 @default.
• W2111418547 cites W2050212558 @default.
• W2111418547 cites W2051754212 @default.
• W2111418547 cites W2051990957 @default.
• W2111418547 cites W2052667799 @default.
• W2111418547 cites W2055944515 @default.
• W2111418547 cites W2058336733 @default.
• W2111418547 cites W2061637970 @default.
• W2111418547 cites W2069539171 @default.
• W2111418547 cites W2071308567 @default.
• W2111418547 cites W2079114759 @default.
• W2111418547 cites W2081281265 @default.
• W2111418547 cites W2085570688 @default.
• W2111418547 cites W2101492969 @default.
• W2111418547 cites W2112823908 @default.
• W2111418547 cites W2113659564 @default.
• W2111418547 cites W2119789736 @default.
• W2111418547 cites W2122580013 @default.
• W2111418547 cites W2123081781 @default.
• W2111418547 cites W2125578752 @default.
• W2111418547 cites W2133725650 @default.
• W2111418547 cites W2143212753 @default.
• W2111418547 cites W2145205801 @default.
• W2111418547 cites W2146259724 @default.
• W2111418547 cites W2149172873 @default.
• W2111418547 cites W2165229392 @default.
• W2111418547 cites W2313494716 @default.
• W2111418547 cites W3099245099 @default.
• W2111418547 cites W3101867971 @default.
• W2111418547 cites W4246565490 @default.
• W2111418547 cites W4249042008 @default.
• W2111418547 cites W4290784459 @default.
• W2111418547 cites W4302071094 @default.
• W2111418547 doi "https://doi.org/10.1111/j.1365-2966.2009.15005.x" @default.
• W2111418547 hasPublicationYear "2009" @default.
• W2111418547 type Work @default.
• W2111418547 sameAs 2111418547 @default.
• W2111418547 citedByCount "42" @default.
• W2111418547 countsByYear W21114185472012 @default.
• W2111418547 countsByYear W21114185472013 @default.
• W2111418547 countsByYear W21114185472014 @default.
• W2111418547 countsByYear W21114185472015 @default.
• W2111418547 countsByYear W21114185472016 @default.
• W2111418547 countsByYear W21114185472017 @default.
• W2111418547 countsByYear W21114185472018 @default.
• W2111418547 countsByYear W21114185472019 @default.
• W2111418547 countsByYear W21114185472020 @default.
• W2111418547 countsByYear W21114185472021 @default.
• W2111418547 countsByYear W21114185472022 @default.
• W2111418547 crossrefType "journal-article" @default.
• W2111418547 hasAuthorship W2111418547A5010037298 @default.
• W2111418547 hasBestOaLocation W21114185471 @default.
• W2111418547 hasConcept C120665830 @default.
• W2111418547 hasConcept C121332964 @default.
• W2111418547 hasConcept C1276947 @default.
• W2111418547 hasConcept C150739758 @default.
• W2111418547 hasConcept C150846664 @default.
• W2111418547 hasConcept C165129702 @default.
• W2111418547 hasConcept C180205008 @default.
• W2111418547 hasConcept C198785896 @default.
• W2111418547 hasConcept C204843146 @default.
• W2111418547 hasConcept C38615331 @default.
• W2111418547 hasConcept C44870925 @default.
• W2111418547 hasConcept C4839761 @default.
• W2111418547 hasConcept C54002840 @default.
• W2111418547 hasConcept C68271606 @default.
• W2111418547 hasConceptScore W2111418547C120665830 @default.
• W2111418547 hasConceptScore W2111418547C121332964 @default.
• W2111418547 hasConceptScore W2111418547C1276947 @default.

• next