Peculiarities of the abundance of chemical elements in the atmosphere of PMMR23-red supergiant in the Small Magellanic Cloud due to interstellar gas accretion
Crossref DOI link: https://doi.org/10.3103/S0884591317050075
Published Online: 2017-11-04
Published Print: 2017-09
Update policy: https://doi.org/10.1007/springer_crossmark_policy
Yushchenko, A. V.
Gopka, V. F.
Shavrina, A. V.
Yushchenko, V. A.
Vasileva, S. V.
Andrievsky, S. M.
Raikov, A. A.
Kim, S.
Rittipruk, P.
Jeong, Y.
Kang, Y.-W.
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