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- W3092134415 endingPage "A34" @default.
- W3092134415 startingPage "A34" @default.
- W3092134415 abstract "The present work presents our efforts at identifying new mercury-manganese (HgMn/CP3) stars using spectra obtained with the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST). Suitable candidates were searched for among pre-selected early-type spectra from LAMOST DR4 using a modified version of the MKCLASS code that probes several Hg II and Mn II features. The spectra of the resulting 332 candidates were visually inspected. Using parallax data and photometry from Gaia DR2, we investigated magnitudes, distances from the Sun, and the evolutionary status of our sample stars. We also searched for variable stars using diverse photometric survey sources. We present 99 bona fide CP3 stars, 19 good CP3 star candidates, and seven candidates. Our sample consists of mostly new discoveries and contains, on average, the faintest CP3 stars known (peak distribution 9.5 < G < 13.5 mag). All stars are contained within the narrow spectral temperature-type range from B6 to B9.5, in excellent agreement with the expectations and the derived mass estimates (2.4 < M(Sun) < 4 for most objects). Our sample stars are between 100 Myr and 500 Myr old and cover the whole age range from zero-age to terminal-age main sequence. They are almost homogeneously distributed at fractional ages on the main sequence < 80%, with an apparent accumulation of objects between fractional ages of 50% to 80%. We find a significant impact of binarity on the mass and age estimates. Eight photometric variables were discovered, most of which show monoperiodic variability in agreement with rotational modulation. Together with the recently published catalogue of APOGEE CP3 stars, our work significantly increases the sample size of known Galactic CP3 stars, paving the way for future in-depth statistical studies." @default.
- W3092134415 created "2020-10-15" @default.
- W3092134415 creator A5001011240 @default.
- W3092134415 creator A5027393390 @default.
- W3092134415 creator A5057395448 @default.
- W3092134415 date "2021-01-01" @default.
- W3092134415 modified "2023-09-27" @default.
- W3092134415 title "New mercury-manganese stars and candidates from LAMOST DR4" @default.
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- W3092134415 cites W1482137935 @default.
- W3092134415 cites W1561585778 @default.
- W3092134415 cites W161266970 @default.
- W3092134415 cites W1636197668 @default.
- W3092134415 cites W1785844464 @default.
- W3092134415 cites W1844214368 @default.
- W3092134415 cites W1951740504 @default.
- W3092134415 cites W1965781205 @default.
- W3092134415 cites W1979379324 @default.
- W3092134415 cites W1983071030 @default.
- W3092134415 cites W1985027493 @default.
- W3092134415 cites W1992218070 @default.
- W3092134415 cites W1992250918 @default.
- W3092134415 cites W1994885868 @default.
- W3092134415 cites W2006066864 @default.
- W3092134415 cites W2030708076 @default.
- W3092134415 cites W2064778606 @default.
- W3092134415 cites W2070508637 @default.
- W3092134415 cites W2086901362 @default.
- W3092134415 cites W2090434735 @default.
- W3092134415 cites W2100832610 @default.
- W3092134415 cites W2116058788 @default.
- W3092134415 cites W2126393949 @default.
- W3092134415 cites W2132963711 @default.
- W3092134415 cites W2134965427 @default.
- W3092134415 cites W2140137154 @default.
- W3092134415 cites W2152046739 @default.
- W3092134415 cites W2153493651 @default.
- W3092134415 cites W2155488926 @default.
- W3092134415 cites W2161912202 @default.
- W3092134415 cites W2184417792 @default.
- W3092134415 cites W2275237310 @default.
- W3092134415 cites W2316557049 @default.
- W3092134415 cites W2344177969 @default.
- W3092134415 cites W2345054490 @default.
- W3092134415 cites W2478335584 @default.
- W3092134415 cites W2482914538 @default.
- W3092134415 cites W2560018763 @default.
- W3092134415 cites W2566258400 @default.
- W3092134415 cites W2593658420 @default.
- W3092134415 cites W2761986865 @default.
- W3092134415 cites W2769417240 @default.
- W3092134415 cites W2784067869 @default.
- W3092134415 cites W2798336535 @default.
- W3092134415 cites W2883752394 @default.
- W3092134415 cites W2890521736 @default.
- W3092134415 cites W2899911787 @default.
- W3092134415 cites W2968888645 @default.
- W3092134415 cites W2997731771 @default.
- W3092134415 cites W3011221771 @default.
- W3092134415 cites W3015556242 @default.
- W3092134415 cites W3016560144 @default.
- W3092134415 cites W3034078400 @default.
- W3092134415 cites W3098643748 @default.
- W3092134415 cites W3098986277 @default.
- W3092134415 cites W3099057661 @default.
- W3092134415 cites W3101187304 @default.
- W3092134415 cites W3101191700 @default.
- W3092134415 cites W3101761967 @default.
- W3092134415 cites W3102052121 @default.
- W3092134415 cites W3102626616 @default.
- W3092134415 cites W3102784118 @default.
- W3092134415 cites W3103095396 @default.
- W3092134415 cites W3103645137 @default.
- W3092134415 cites W3103663129 @default.
- W3092134415 cites W3105226892 @default.
- W3092134415 cites W3105390848 @default.
- W3092134415 cites W3105621264 @default.
- W3092134415 cites W3105934001 @default.
- W3092134415 cites W3106162659 @default.
- W3092134415 cites W3106457814 @default.
- W3092134415 cites W3116209121 @default.
- W3092134415 cites W3124690141 @default.
- W3092134415 cites W3124789757 @default.
- W3092134415 cites W4211202475 @default.
- W3092134415 cites W4239762937 @default.
- W3092134415 cites W4288083596 @default.
- W3092134415 cites W4289813091 @default.
- W3092134415 cites W4292400099 @default.
- W3092134415 cites W4297723886 @default.
- W3092134415 cites W4299493560 @default.
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- W3092134415 doi "https://doi.org/10.1051/0004-6361/202038847" @default.
- W3092134415 hasPublicationYear "2021" @default.
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