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Atmospheres of six red giants
CCD spectrograms are used to analyse abundances (20 chemical elements) in the atmosphere of six giants. -
Energy distribution in giants and supergiants.
The energy distributions for 27 giants and supergiants of the M spectral type are presented in the region of 3200-7600{AA} with the step of 50{AA}. The observations were made in... -
Equivalent widths for 54 red giants
We present equivalent widths for 54 red giants in five globular clusters, and compare the data with those of other workers. This material will form the basis for subsequent... -
M2FS & Hectochelle spectra of dSph in the MW halo
We present spectroscopic data for 16369 stellar targets within and/or toward 38 dwarf spheroidal galaxies and faint star clusters within the Milky Way halo environment. All... -
Abundance measurements in M15 RGB stars
Large-scale surveys will provide spectroscopy for ~50 million resolved stars in the Milky Way and Local Group. However, these data will have a high degree of heterogeneity and... -
LAMOST DR9 M-giant stars value-added cat.
In this work, we update the catalog of M-giant stars from the low-resolution spectra of the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) Data Release 9.... -
NEOWISE variability of Gaia Herbig Ae/Be & Be stars
Light variability is an essential attribute of young stellar objects (YSOs) at the pre-main-sequence (PMS) stage, which can be treated as an indicator to trace star formation.... -
Milky Way Mira variable stars from OGLE
We present a collection of 65,981 Mira-type variable stars found in the Optical Gravitational Lensing Experiment (OGLE) project database. Two-thirds of our sample (40,356... -
O-rich and C-rich AGB stars in our Galaxy
We present a new catalog of 11209 O-rich asymptotic giant branch (AGB) stars and 7172 C-rich AGB stars in our Galaxy, identifying more AGB stars in the bulge component and... -
Survey of SiO maser emission in oxygen-rich stars
Circumstellar environments of oxygen-rich stars are among the strongest SiO maser emitters. Physical processes such as collisions, infrared pumping, and overlaps favor the... -
Mira-like variables from the KELT survey
We present a sample of 4132 Mira-like variables (red variables with long periods and high amplitudes) in the Kilodegree Extremely Little Telescope (KELT) survey. Of these, 376... -
Vanadium transitions in the spectrum of Arcturus
We derive a new abundance for vanadium in the bright, mildly metal-poor red giant Arcturus. This star has an excellent high-resolution spectral atlas and well-understood... -
Mira stars discovered in LAMOST DR4
Based on an extensive spectral study of a photometrically confirmed sample of Mira variables, we find a relationship between the relative Balmer emission-line strengths and... -
The populations of Carina. II. Abundances
Chemical abundances are presented for 19 elements in a sample of 63 red giants in the Carina dwarf spheroidal galaxy (dSph), based on homogeneous 1D/LTE model atmosphere... -
Carbon stars from LAMOST DR2 data
In this work, we present the new catalog of carbon stars from the LAMOST DR2 catalog. In total, 894 carbon stars are identified from multiple line indices measured from the... -
Ca,by photometry in globular clusters. I. M22
We investigate the multiple stellar populations in one of the peculiar globular clusters (GCs), M22, using new ground-based wide-field Ca by and Hubble Space Telescope... -
Fundamental stellar parameters in 47 Tucanae
Fundamental parameters and time evolution of mass loss are investigated for post-main-sequence stars in the Galactic globular cluster 47 Tucanae (NGC 104). This is accomplished... -
EWs of eta Carinae from ~30yrs sp. monitoring
Eta Carinae ({eta} Car) exhibits a unique set of P Cygni profiles with both broad and narrow components. Over many decades, the spectrum has changed-there has been an increase... -
Low-luminosity Kepler red giants analysis
We present measurements of the dipole mode asymptotic period spacing ({Delta}{Pi}1), the coupling factor between the p- and g-modes (q), the g-mode phase offset ({epsilon}g),... -
Improved stellar parameters of Kepler RGB stars
This paper reports the estimated stellar parameters of 1153 Kepler red giant branch stars determined with asteroseismic modeling. We use radial-mode oscillation frequencies,...
