Sep 18 @ 7:30 pm – 9:00 pm Atkinson Recital Hall, NMSU
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Oct 2 @ 3:15 pm – 4:15 pm BX102
Insights into Binary Stars, Stellar Winds, and Astrophysical Plasmas from X-ray Observations of Planetary Nebulae Rodolfo Montez Jr., Vanderbilt University   Share this:TweetPrint
Oct 16 @ 3:15 pm – 4:15 pm BX102
Why Space Weather Matters and How Forecasting Will Improve in the DSCOVR Era Doug Biesecker, NOAA/NWS/Space Weather Prediction Center Space Weather is a growing enterprise, with growing recognition of its importance inside and outside government. ...
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Dec 4 @ 3:15 pm – 4:15 pm BX102
On the Edge: Exoplanets with Orbital Periods Shorter Than a Peter Jackson Movie Brian Jackson, Boise State Univeristy From wispy gas giants to tiny rocky bodies, exoplanets with orbital periods of several days and less...
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Feb 12 @ 3:15 pm – 4:15 pm BX102
Magnetic Influences on Coronal Heating and the Solar Wind Lauren Woolsey, Harvard University   Abstract The physical mechanism(s) that generate and accelerate the solar wind have not been conclusively determined after decades of study, though not...
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May 12 @ 3:00 pm – 4:00 pm Dominici106
Evolution of Dwarf Galaxy Properties in Local Group Environments Kenz Arraki, NMSUShare this:TweetPrint
May 31 @ 3:00 pm – 4:00 pm Dominici106
Ages and Abundance of Local Stellar Populations Diane Feuillet, NMSUShare this:TweetPrint
Oct 28 @ 3:15 pm – 4:15 pm Biology Annex 102
Star formation in the vicinity of the supermassive black hole at the Galactic Centre Dr. Mark Wardle, Macquarie University The disruptive tidal field near supermassive black holes overcomes the self-gravity of objects that are less...
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Jun 27 @ 2:30 pm – 3:30 pm Domenici Hall 102
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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Jul 3 @ 2:00 pm – 3:00 pm
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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Sep 1 @ 3:15 pm – 4:15 pm BX102
A Faint Flux-Limited LAE Sample at z = 0.3 Isak Wold, UT Austin Observational surveys of Lya emitters (LAEs) have proven to be an efficient method to identify and study large numbers of galaxies over...
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Sep 20 @ 3:00 pm – 4:15 pm Business College 103
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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Mar 28 @ 3:15 pm – 4:15 pm Science Hall 109
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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Oct 19 @ 3:15 pm – 4:15 pm BX102
Understanding How Galaxies Reionized the Universe  Sanchayeeta Borthakur, Arizona State University Identifying the population of galaxies that was responsible for the reionization of the universe is a long-standing quest in astronomy. While young stars can...
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Jan 23 @ 3:00 pm – 4:00 pm
Extinction Mapping and Dust-to-Gas Ratios of Nearby Galaxies Lauren Kahre, NMSU We present a study of the dust{to{gas ratios in 31 nearby (D > 10 Mpc) galaxies. Using Hubble Space Telescope broad band WFC3/UVIS UV...
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Feb 20 @ 3:15 pm – 4:15 pm Domenici Hall
The AAVSO Program: A Resource for Variable Star Research Stella Kafka, AAVSO The AAVSO was formed in 1911 as a group of US-based amateur observers obtaining data in support of professional astronomy projects. Now, it...
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Mar 5 @ 7:30 pm – 8:45 pm ASNMSU Center for the Arts
Dr. Janna Levin Barnard College   Info here:    Share this:TweetPrint
Dec 6 @ 3:15 pm – 4:15 pm BX102
Revealing reionization with the thermal history of the intergalactic medium Elisa Boera, SISSA Trieste During hydrogen reionization the UV radiation from the first luminous sources injected vast amount of energy into the intergalactic medium, photo-heating...
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