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- W4214546098 abstract "The results of new spectral and photometric observations of the poorly studied S-star CSS 1102 are presented. Accordingto the analysis of spectra, CSS 1102 was classified as a symbiotic star. We observed HI, HeI and [NeIII] emission linesin both spectra of the star. The absorption spectrum demonstrates the prominent molecular bands of TiO, ZrO andYO. The system consists of a cold component that is a zirconium star of spectral type S4.5/2, a hot component with40000 K < T hot < 55000 K, and a nebula. Photometric monitorings in the B band showed the existence of a flickeringeffect with different periods in CSS 1102. This variability may be associated with emission of an accretion disk in CSS 1102system." @default.
- W4214546098 created "2022-03-02" @default.
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- W4214546098 date "2022-02-22" @default.
- W4214546098 modified "2023-09-27" @default.
- W4214546098 title "Confirmation of the symbiotic nature of CSS 1102 on the basis of spectral and photometric observations carried out at the CMO SAI MSU" @default.
- W4214546098 doi "https://doi.org/10.51194/vak2021.2022.1.1.187" @default.
- W4214546098 hasPublicationYear "2022" @default.
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