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High-resolution spectroscopy and spectropolarimetry of selected delta Sct pulsating variables
Joshi S., Semenko E., Moiseeva A., Sharma K., Joshi Y.C., Sachkov M., Singh H.P., Yerra B.K.
The combination of photometry, spectroscopy and spectropolarimetry of the chemically peculiar stars
An abundance analysis of the single-lined spectroscopic binaries with barium stars-like orbital elements: I. Analysis and results
Začs L., Musaev F., Bikmaev I., Alksnis O.
(primaries) in barium star like binary systems with WD component have chemical peculiarities (very slight
Analysis of fundamental parameters for V477 Lyr
Shimansky V., Pozdnyakova S., Borisov N., Bikmaev I., Galeev A., Sakhibullin N., Spiridonova O.
We analyze the photometric and spectroscopic observations of the young pre-cataclysmic variable
Lithium on the surface of cool magnetic CP stars. II. Spectrum analysis of HD 83368 and HD 60435 with lithium spots
Shavrina A., Polosukhina N., Zverko J., Mashonkina L., Khalack V., Ziznovský J., Hack M., Tsymbal V., North P., Vygonec V.
are compared with HD 83368, the other star with lines of lithium remarkably variable in intensity
An abundance analysis of the single-lined spectroscopic binaries with barium stars-like orbital elements: II. The spectroscopic data
Začs L., Alksnis O., Musaev F., Bikmaev I., Galazutdinov G.
non-variable barium stars, and two standards. All binary systems contain an unseen low-mass component
An abundance analysis of the single-lined spectroscopic binaries with barium stars-like orbital elements: I. Analysis and results
Začs L., Musaev F., Bikmaev I., Alksnis O.
(primaries) in barium star like binary systems with WD component have chemical peculiarities (very slight
An abundance analysis of the single-lined spectroscopic binaries with barium stars-like orbital elements: II. The spectroscopic data
Začs L., Alksnis O., Musaev F., Bikmaev I., Galazutdinov G.
non-variable barium stars, and two standards. All binary systems contain an unseen low-mass component
Outstanding X-ray emission from the stellar radio pulsar CU Virginis
Robrade J., Oskinova L., Schmitt J., Leto P., Trigilio C.
© ESO 2018. Context. Among the intermediate-mass magnetic chemically peculiar (MCP) stars, CU Vir
Eu III oscillator strengths and Europium abundances in Ap stars
Mashonkina L., Ryabtsev A., Ryabchikova T.
of hot peculiar stars (α2 CVn is a typical representative) and cool peculiar stars (β CrB is a typical
Analysis of fundamental parameters for V477 Lyr
Shimansky V., Pozdnyakova S., Borisov N., Bikmaev I., Galeev A., Sakhibullin N., Spiridonova O.
We analyze the photometric and spectroscopic observations of the young pre-cataclysmic variable

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