FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3105472430> ?p ?o ?g. }

• W3105472430 endingPage "70" @default.
• W3105472430 startingPage "70" @default.
• W3105472430 abstract "This study is an attempt to determine the metallicities of WUMa-type binary stars using spectroscopy. ~4,500 spectra collected at the David Dunlap Observatory were subject to the same Broadening Function processing to determine the combined line strength in the spectral window centered on the MgI triplet (5080-5285A). Individual integrated BF's were phase averaged to derive a single line-strength indicator. The sample was limited to 90 EW binaries with the strict phase-constancy of colors and without spectral contamination by companions. The best defined results were obtained for a F-type sub-sample (0.32<(B-V)0<0.62) of 52 stars for which the BF strengths could be interpolated in the model predictions. The metallicities, [M/H], for the F-type sub-sample indicate abundances roughly similar to the solar [M/H], but with a large scatter which is partly due to combined random and systematic errors. Because of a color trend resulting from limitations in our approach, we set the scale of metallicities to correspond to that derived from the m_1 index of the Stromgren photometry for F-type binaries. The trend-adjusted [M/H]1 are distributed within -0.65<[M/H]1<+0.50, with the spread reflecting genuine metallicity differences between stars. One half of the F-sub-sample binaries have [M/H]1 within -0.37<[M/H]1 +0.10, a median of -0.04 and a mean of -0.10, with a tail towards low metallicities, and a possible bias against very high metallicities. A parallel study of kinematic data, utilizing the most reliable and recently obtained proper motion and radial velocity data for 78 stars of the full sample, shows that the F-type sub-sample binaries have similar kinematic properties to solar neighborhood, thin-disk dwarfs with ages about 3 - 5.5 Gyr. The F-type binaries which appear to be older than the rest tend to have systematically smaller mass-ratios than most of the EW binaries of the same period." @default.
• W3105472430 created "2020-11-23" @default.
• W3105472430 creator A5058962721 @default.
• W3105472430 creator A5061729160 @default.
• W3105472430 creator A5071263036 @default.
• W3105472430 date "2013-08-14" @default.
• W3105472430 modified "2023-10-18" @default.
• W3105472430 title "SPECTROSCOPIC METALLICITY DETERMINATIONS FOR W UMa-TYPE BINARY STARS" @default.
• W3105472430 cites W1561821896 @default.
• W3105472430 cites W1584002683 @default.
• W3105472430 cites W1618769467 @default.
• W3105472430 cites W1619205399 @default.
• W3105472430 cites W1670318221 @default.
• W3105472430 cites W188239022 @default.
• W3105472430 cites W1972810172 @default.
• W3105472430 cites W1978509626 @default.
• W3105472430 cites W1988033481 @default.
• W3105472430 cites W1990554638 @default.
• W3105472430 cites W199200718 @default.
• W3105472430 cites W1993480829 @default.
• W3105472430 cites W2000392429 @default.
• W3105472430 cites W2006147999 @default.
• W3105472430 cites W2009056029 @default.
• W3105472430 cites W2018649059 @default.
• W3105472430 cites W2021105357 @default.
• W3105472430 cites W2024909325 @default.
• W3105472430 cites W2025520753 @default.
• W3105472430 cites W2025837743 @default.
• W3105472430 cites W2030124160 @default.
• W3105472430 cites W2031043816 @default.
• W3105472430 cites W2035704816 @default.
• W3105472430 cites W2038063157 @default.
• W3105472430 cites W2041752480 @default.
• W3105472430 cites W2043842882 @default.
• W3105472430 cites W2046192500 @default.
• W3105472430 cites W2067530731 @default.
• W3105472430 cites W2068843564 @default.
• W3105472430 cites W2068905762 @default.
• W3105472430 cites W2069161247 @default.
• W3105472430 cites W2072538366 @default.
• W3105472430 cites W2072621059 @default.
• W3105472430 cites W2072762311 @default.
• W3105472430 cites W2073488875 @default.
• W3105472430 cites W2074544151 @default.
• W3105472430 cites W2078330210 @default.
• W3105472430 cites W2085171875 @default.
• W3105472430 cites W2088042527 @default.
• W3105472430 cites W2092097624 @default.
• W3105472430 cites W2092098800 @default.
• W3105472430 cites W2111817932 @default.
• W3105472430 cites W2119387732 @default.
• W3105472430 cites W2124186900 @default.
• W3105472430 cites W2132530152 @default.
• W3105472430 cites W2135812749 @default.
• W3105472430 cites W2137744066 @default.
• W3105472430 cites W2142220522 @default.
• W3105472430 cites W2143845084 @default.
• W3105472430 cites W2152296757 @default.
• W3105472430 cites W2153222874 @default.
• W3105472430 cites W2160299852 @default.
• W3105472430 cites W2162222062 @default.
• W3105472430 cites W2164355923 @default.
• W3105472430 cites W2165506425 @default.
• W3105472430 cites W2168626251 @default.
• W3105472430 cites W3009699307 @default.
• W3105472430 cites W3098315300 @default.
• W3105472430 cites W3098530119 @default.
• W3105472430 cites W3099623684 @default.
• W3105472430 cites W3100509646 @default.
• W3105472430 cites W3101320803 @default.
• W3105472430 cites W3102357848 @default.
• W3105472430 cites W3104411766 @default.
• W3105472430 cites W3104559670 @default.
• W3105472430 cites W3104913648 @default.
• W3105472430 cites W3104962767 @default.
• W3105472430 cites W3105257296 @default.
• W3105472430 cites W3105429990 @default.
• W3105472430 cites W3105524264 @default.
• W3105472430 cites W3121530766 @default.
• W3105472430 cites W3122138144 @default.
• W3105472430 cites W3122591886 @default.
• W3105472430 cites W4244350690 @default.
• W3105472430 cites W4249503389 @default.
• W3105472430 cites W4292385952 @default.
• W3105472430 cites W4294843887 @default.
• W3105472430 cites W2008413306 @default.
• W3105472430 doi "https://doi.org/10.1088/0004-6256/146/3/70" @default.
• W3105472430 hasPublicationYear "2013" @default.
• W3105472430 type Work @default.
• W3105472430 sameAs 3105472430 @default.
• W3105472430 citedByCount "25" @default.
• W3105472430 countsByYear W31054724302014 @default.
• W3105472430 countsByYear W31054724302015 @default.
• W3105472430 countsByYear W31054724302016 @default.
• W3105472430 countsByYear W31054724302017 @default.
• W3105472430 countsByYear W31054724302018 @default.
• W3105472430 countsByYear W31054724302019 @default.
• W3105472430 countsByYear W31054724302020 @default.

• next