Affiliate Member
Yahira Mendoza
Membership since:
2025
Field of activity:
Other Memberships/Affiliations
Observátorio do Valongo, Universidade Federal do Rio de Janeiro
Degrees:
2022
Undergraduate Physics
Publications resulting from Research
Times of maximum of KZ Hya from OACS -UNAH
A pulsating variable star is one whose brightness changes periodically due to the expansion and contraction of the surface layers of the star. Several times of maximum light can be obtained in brief observations of SX Phoenicis variable stars due to their short periods of pulsation (P ~ 1:0 - 1:75 h). We report three new times of maximum light of SX Phoenicis star KZ Hya obtained from photometric observations made on the night of April 5-6, 2019 from the Observatorio Astronómico Centroaméricano de Suyapa (OACS) of the Universidad Nacional Autónoma de Honduras
A pulsating variable star is one whose brightness changes periodically due to the expansion and contraction of the surface layers of the star. Several times of maximum light can be obtained in brief observations of SX Phoenicis variable stars due to their short periods of pulsation (P ~ 1:0 - 1:75 h). We report three new times of maximum light of SX Phoenicis star KZ Hya obtained from photometric observations made on the night of April 5-6, 2019 from the Observatorio Astronómico Centroaméricano de Suyapa (OACS) of the Universidad Nacional Autónoma de Honduras
12 Escuela de Verano en Astrofísica
2025
Instituto de Radioastronomía y Astrofísica, Universidad Nacional Autónoma de México, MéxicoWomen in physics in developing countries
2025
International Conference on Women in Physics, International Union of Pure and Applied Physics, AustraliaData Professionalism
2025
International Conference on Women in Physics, International Union of Pure and Applied Physics, Australia