Evolution of Dwarf Galaxy Properties in Local Group Environments Kenz Arraki, NMSUShare this:TweetPrint
Ages and Abundance of Local Stellar Populations Diane Feuillet, NMSUShare this:TweetPrint
The Orbital and Planetary Phase Variations of Jupiter-Sized Planets: Characterizing Present and Future Giants Laura Mayorga, NMSU It is commonly said that exoplanet science is 100 years behind planetary science. While we may be able...
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The Vulture Survey of MgII and CIV Absorbers: Feasting on the Bones of Spectra Left to Die Nigel Mathes, NMSU Abstract: We present detailed measurements of the absorption properties and redshift evolution of MgII and...
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Asteroseismology of Red Giants: The Detailed Modeling of Red Giants in Eclipsing Binary Systems Jean McKeever, NMSU Asteroseismology is an invaluable tool that allows one to peer into the inside of a star and know...
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Seismic Inferences of Gas Giant Planets: Excitation & Interiors Ethan Dederick, NMSU Seismology has been the premier tool of study for understanding the interior structure of the Earth, the Sun, and even other stars. In...
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Dr. Janna Levin Barnard College Info here: https://honors.nmsu.edu/news/events/speakers-series/ Share this:TweetPrint
Join us for the inaugural Las Cruces chapter of Astronomy on Tap! Join local astronomers from the NMSU Astronomy Department for a night of fun, accessible space-related presentations, games, and prizes. Please RSVP on the...
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Join us for the second round of Astronomy on Tap: Las Cruces! Join local astronomers from the NMSU Astronomy Department for a night of fun, accessible space-related presentations, games, and prizes. You can access the...
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Dependence upon Obliquity of the Formation of Martian PLD Vertical Structure Jeremy Emmett, NMSU Mars’ polar layered deposits (PLD) are comprised of layers of varying dust-to-water ice volume mixing ratios (VMR) that are thought to...
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H-Band Spectroscopy of Exotic, Massive Stars Drew Chojnowski, NMSU We report on spectroscopy of exotic B-type emission line (Be) stars and chemically peculiar (CP) stars in the near-infrared (NIR) H-band, using data provided by the...
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