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Study of the Carbon Star T Draconis
DOI: 10.1134/S1063773724600176 Bibcode: 2024AstL...50...53T

Tatarnikov, A. M.; Shenavrin, V. I.; Zheltoukhov, S. G. +2 more

We present the results of the infrared photometric observations in the $JHKLM$ bands and infrared spectroscopic observations in the range 1-2.5 $µ$m for the carbon Mira star T Dra performed from 2019 to 2023. An analysis of the photometric observations shows the presence of both pulsational brightness fluctuations with an amplitude falling f…

2024 Astronomy Letters
AKARI Gaia ISO 2
Multicolor Photometry and Peculiarities of the Spectrum for the post-AGB Candidate AU Vulpeculae (IRAS 20160+2734)
DOI: 10.1134/S1063773721070057 Bibcode: 2021AstL...47..485I

Esipov, V. F.; Ikonnikova, N. P.; Tatarnikov, A. M. +7 more

We present the results of a UBVRcIc and JHKLM photometric monitoring campaign conducted in 2016-2020, low-resolution spectroscopy, and an analysis of the ASAS-3 and ASAS-SN photometric data for the semiregular variable and post-AGB candidate AU Vul (IRAS 20160+2734). The star is shown to experience quasi-periodic brightness oscillations with a var…

2021 Astronomy Letters
AKARI Gaia 0
Estimates of Extragalactic Background and Confusion Noise Parameters for the Millimetron Telescope
DOI: 10.1134/S1063773720050023 Bibcode: 2020AstL...46..298E

Pilipenko, S. V.; Ermash, A. A.; Lukash, V. N.

The sensitivity of future far-infrared telescopes, such as Millimetron, will be limited by the confusion noise produced by distant galaxies. We have constructed a model of the cosmic infrared background whose main goal is to investigate the confusion noise parameters. The model is based on the publicly accessible eGALICS simulation. For each galax…

2020 Astronomy Letters
AKARI 6