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Mexican astronomer From Wikipedia, the free encyclopedia
Yolanda Gómez Castellanos (1962–2012) was a Mexican astronomer who studied interstellar clouds including planetary nebulae and compact H II regions.[1][2] She became known for the discovery of water vapor through emissions from astrophysical masers associated with OH/IR stars and planetary nebulae,[1][2] evidence for the extremely recent formation of the associated nebula.[3]
Gómez was born in Mexico City,[4][5] in 1962.[5][6] She studied physics at the National Autonomous University of Mexico (UNAM), earning a bachelor's degree in 1985 and completing her doctorate in 1990.[4]
After postdoctoral research at the Harvard–Smithsonian Center for Astrophysics, she became a researcher at UNAM in 1993, first in the Institute of Astronomy and after 2001 as a founding member of the Center for Radio Astronomy and Astrophysics of the Morelia campus of UNAM.[2][5]
Gómez was a member of the Mexican Academy of Sciences.[7] In 2005, UNAM gave her the Sor Juana Inés de la Cruz Recognition.[5] In 2008 the government of Michoacán gave her the State Prize for the Dissemination of Science and Technology.[6]
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