Based on the TESS (Transiting Exoplanet Survey Satellite) phase dependent light curves, we confirm the eclipsing type variability nature for two G – type dwarfs: TYC 1417-891-1 and TYC 1478-742-1. Both objects show EA (Algol – type) light curves morphology. Orbital period for TYC 1417-891-1 is P ≈ 8.0 day and for TYC 1478-742-1, P ≈ 13.6 day. We present Gaia EDR3 and TESS catalogue important physical parameters as well as LAMOST spectra. Both objects are relatively bright and are located at a distance of 260.59 (±3.21) pc (TYC 1417-891-1) and 117.42 (±0.74) pc (TYC 1478-742-1). The TESS light curve of TYC 1478-742-1 show also flares as well. We discuss possible nature of the secondary and faint objects around these stars.
oai:arar.sci.am:361050
ՀՀ ԳԱԱ Հիմնարար գիտական գրադարան
Aug 1, 2024
Jul 10, 2023
20
https://arar.sci.am/publication/390320
Edition name | Date |
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Gigoyan, K. K., TYC 1417-891-1 and TYC 1478-742-1: Eclipsing variable stars. The Gaia EDR3 and TESS photometric data | Aug 1, 2024 |
Gigoyan, K. K. Gigoyan, K. S. Sarkissian, A. Meftah, M. Kostandyan, G. R. Rahmatullaeva, F. Գլխավոր խմբ․՝ Վ․ Հ․ Համբարձումյան (1965-1987) Լ․ Վ․ Միրզոյան (1988-1999) Դ․ Մ․ Սեդրակյան (2000-2017) Ա․ Գ․ Նիկողոսյան (2018-)
Kostandyan, G. R. Gigoyan, K. S. Gigoyan, K. K.
Gigoyan, K. S. Mickaelian, A. M. Kostandyan, G. R.
Mickaelian, A. M. Gigoyan, K. S. Mikayelyan, G. A. Paronyan, G. M. Gyulzadyan, M. V. Kostandyan, G. R.
Mickaelian, A. M. Gigoyan, K. S. Gyulzadyan, M. V. Paronyan, G. M. Abrahamyan, H. V. Andreasyan, H. R. Azatyan, N. M. Kostandyan, G. R. Samsonyan, A. L. Mikayelyan, G. A. Farmanyan, S. V. Harutyunyan, V. L.
K. S. Gigoyan G. R. Kostandyan K. K. Gigoyan F. Zamkotsian A. Sarkissian Գլխավոր խմբ․՝ Վ․ Հ․ Համբարձումյան (1965-1987) Լ․ Վ․ Միրզոյան (1988-1999) Դ․ Մ․ Սեդրակյան (2000-2017) Ա․ Գ․ Նիկողոսյան (2018-)