First detection of 22 GHz H2O masers in TX Camelopardalis
Se-Hyung Cho, Jaeheon Kim, and Youngjoo Yun

TL;DR
This study reports the first detection of 22 GHz H2O masers in TX Camelopardalis, providing insights into maser behavior and stellar atmosphere conditions through simultaneous multi-frequency observations.
Contribution
It presents the first detection of H2O masers in TX Cam and analyzes their variability and velocity shifts relative to SiO masers across multiple epochs.
Findings
H2O masers detected near stellar velocity at five epochs.
H2O maser intensities are weaker than SiO masers.
Velocity shifts of SiO masers vary with phase.
Abstract
Simultaneous time monitoring observations of HO , SiO = 1--0, 2--1, 3--2, and SiO = 0, = 1--0 lines were carried out in the direction of the Mira variable star TX Cam with the Korean VLBI Network single dish radio telescopes. For the first time, the HO maser emission from TX Cam was detected near the stellar velocity at five epochs from April 10, 2013 ( = 3.13) to June 4, 2014 ( = 3.89) including minimum optical phases. The intensities of HO masers are very weak compared to SiO masers. The variation of peak antenna temperature ratios among SiO = 1, = 1--0, = 2--1, and = 3--2 masers is investigated according to their phases. The shift of peak velocities of HO and SiO masers with respect to the stellar velocity is also investigated according to observed optical phases. The HO maser emission occurs…
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