The 2021 Hot-type Symbiotic Outburst of YY Herculis: An Optical Follow-up Study
L. S. Sonith, U. S. Kamath

TL;DR
This study presents a detailed optical follow-up of the 2021 hot-type symbiotic outburst of YY Herculis, analyzing spectral evolution and orbital phase dependence over 1.5 cycles, revealing temperature and luminosity variations.
Contribution
It provides the first comprehensive spectral evolution analysis of the 2021 outburst over a full orbital cycle, highlighting phase-dependent temperature and luminosity changes.
Findings
Outburst temperature: ~1.41 x 10^5 K, luminosity: ~1020 L_sun
Post-outburst temperature: ~1.3 x 10^5 K, luminosity: ~830 L_sun
Confirmed ellipsoidal effect contribution in light curve minima
Abstract
We have followed up on the hot-type classical symbiotic outburst reported in YY Her using the Himalayan Chandra telescope. The outburst coincides with the secondary minima of the system. Approximately 12 similar brightening events have been reported between 1890 and 2020, with only the 1993 outburst being studied spectroscopically. In our study, we monitored the system from 2021 to 2023, covering 1.5 orbital cycles, providing an opportunity to understand the spectral evolution of the outburst over a complete orbital period of YY Her. We found that the temperature and luminosity estimations based on emission line fluxes exhibit orbital phase dependence. The values estimated at phase 0.5, corresponding to the secondary minimum, were the most reliable. The temperature of the hot component is , and the luminosity is …
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Taxonomy
TopicsAstrophysical Phenomena and Observations · Astronomy and Astrophysical Research · Stellar, planetary, and galactic studies
