A plethora of new, magnetic chemically peculiar stars from LAMOST DR4
arXiv:2005.14444 · doi:10.1051/0004-6361/202037750
Abstract
Magnetic chemically peculiar (mCP) stars are important to astrophysics because their complex atmospheres lend themselves perfectly to the investigation of the interplay between such diverse phenomena as atomic diffusion, magnetic fields, and stellar rotation. The present work is aimed at identifying new mCP stars using spectra collected by the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST). Suitable candidates were selected by searching LAMOST DR4 spectra for the presence of the characteristic 5200A flux depression. Spectral classification was carried out with a modified version of the MKCLASS code and the accuracy of the classifications was estimated by comparison with results from manual classification and the literature. Using parallax data and photometry from Gaia DR2, we investigated the space distribution of our sample stars and their properties in the colour-magnitude diagram. Our final sample consists of 1002 mCP stars, most of which are new discoveries (only 59 previously known). Traditional mCP star peculiarities have been identified in all but 36 stars, highlighting the efficiency of the code's peculiarity identification capabilities. The derived temperature and peculiarity types are in agreement with manually derived classifications and the literature. Our sample stars are between 100 Myr and 1 Gyr old, with the majority having masses between 2M(Sun) and 3M(Sun). Our results could be considered as strong evidence for an inhomogeneous age distribution among low-mass (M < 3M(Sun)) mCP stars. We identified several astrophysically interesting objects: two mCP stars have distances and kinematical properties in agreement with halo stars; an eclipsing binary system hosting an mCP star component; and an SB2 system likely comprising of an mCP star and a supergiant component.
62 pages, 24 figures, 10 tables, corrected some typos and minor mistakes; corrected wrong number of stars with absolute parallax errors less than 25%, redundant figure removed
References in corpus (19)
- VOSA: Virtual Observatory SED Analyzer. An application to the Collinder 69 open cluster
- The first WASP public data release
- Weak magnetic fields in Ap/Bp stars: Evidence for a dipole field lower limit and a tentative interpretation of the magnetic dichotomy
- Evolutionary state of magnetic chemically peculiar stars
- Searching for links between magnetic fields and stellar evolution. I. A survey of magnetic fields in open cluster A- and B-type stars with FORS1
- Searching for links between magnetic fields and stellar evolution III. Measurement of magnetic fields in open cluster Ap stars with ESPaDOnS
- Chemically peculiar stars and their temperature calibration
- MOBSTER - II. Identification of rotationally variable A stars observed with \emph{TESS} in Sectors 1 to 4
- Pulsation versus metallicism in Am stars as revealed by LAMOST and WASP
- Theoretical analysis of the atmospheres of CP stars. Effects of the individual abundance patterns
- Gaia's view of the Boo star puzzle
- Doppler imaging of chemical spots on magnetic Ap/Bp stars. Numerical tests and assessment of systematic errors
- Metallic-Line Stars Identified from Low Resolution Spectra of LAMOST DR5
- A Large Sample of Am Candidates from LAMOST Data Release 1
- Exploring the spectral \textit{information content} in the LAMOST medium-resolution survey (MRS)
- The structural evolution of galaxies with both thin and thick discs
- HD 99458: First time ever Ap-type star as a Scuti pulsator in a short period eclipsing binary?
- Surface abundance and the hunt for stratification in chemically peculiar hot subdwarfs: PG 0909+276 and UVO 0512-08
- HD66051, an eclipsing binary hosting a highly peculiar, HgMn-related star
Cited by in corpus (20)
- Stellar labels for hot stars from low-resolution spectra - I. the HotPayne method and results for 330,000 stars from LAMOST DR6
- New mercury-manganese stars and candidates from LAMOST DR4
- Magnetism in High-Mass Stars
- Photometric variability of the LAMOST sample of magnetic chemically peculiar stars as seen by TESS
- Exploring the stellar rotation of early-type stars in the LAMOST Medium-Resolution Survey. II. Statistics
- Magnetic chemically peculiar stars investigated by the Solar Mass Ejection Imager
- An Ap star catalog based on LAMOST DR9
- The detection of magnetic chemically peculiar stars using Gaia BP/RP spectra
- New magnetic chemically peculiar stars and candidates in the ATLAS First Catalog of Variable Stars
- HD 60431, the CP2 star with the shortest rotational period -- Physical parameters and period analysis
- V680 Mon -- a young mercury-manganese star in an eclipsing heartbeat system
- Rotational Velocities of Am and Non-CP Stars based on Kepler and LAMOST DR5
- The astrophysical parameters of chemically peculiar stars from automatic methods
- Exploring the Stellar Rotation of Early-type Stars in the LAMOST Medium-resolution Survey. III. Evolution
- Searching for shell stars in LAMOST DR4 by probing the Fe 42 multiplet lines
- A new sample of super-slowly rotating Ap (ssrAp) stars from the Zwicky Transient Facility survey
- High-velocity CP2 stars in the Galactic halo
- Magnetism in LAMOST CP stars observed by TESS
- Chemically peculiar stars on the pre-main sequence
- A case study of ACV variables discovered in the Zwicky Transient Facility survey