Apr 6 @ 3:15 pm – 4:15 pm
Colloquium Title Sten Hasselquist, NMSU AbstractShare this:TweetPrint
Feb 6 @ 3:15 pm – 4:15 pm
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Feb 11 @ 3:00 pm – 4:00 pm
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Feb 12 @ 3:00 pm – 4:00 pm
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Feb 13 @ 3:15 pm – 4:15 pm
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Feb 17 @ 3:15 pm – 4:15 pm
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Feb 19 @ 1:00 pm – 2:00 pm
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Feb 20 @ 3:15 pm – 4:15 pm
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Feb 26 @ 3:30 pm – 4:30 pm
A Multi-Wavelength Study of the Evolution of Solar Flares Sean Sellers, NMSU Share this:TweetPrint
Mar 13 @ 3:15 pm – 4:15 pm
Galaxy Evolution from Large Surveys of Nearby Resolved Galaxies Karen Masters (Haverford College, Spokesperson for SDSS-IV) Abstract: The morphology of a galaxy provides information on the orbits of stars within it. As such, important clues...
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Mar 20 @ 3:15 pm – 4:15 pm
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Apr 3 @ 3:15 pm – 4:15 pm
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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Apr 17 @ 3:00 pm – 4:00 pm
Evolution of Ionized Interstellar Medium across Cosmic Time Fuyan Bian, European Southern Observatory The ionized interstellar medium (ISM) provides essential information on the star-forming environments, metal enrichment, and underlying ionizing radiation field in galaxies. It...
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Apr 24 @ 9:00 am – 10:00 am
Planet formation in protoplanetary discs around young stars Anders Johansen (Lund University, Sweden) Planets form in protoplanetary discs around young stars as dust and ice particles collide to form larger and larger bodies. I will...
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May 8 @ 3:00 pm – 4:00 pm
Enhancing Time-Dependent Solar Wind Models to Constrain Effects on Non-Magnetized Planetary Atmospherese Sarah Kovac, NMSU The Sun generates a solar wind of particles which propagate throughout the solar system and can be modeled using magnetohydrodynamics...
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May 29 @ 2:30 pm – 3:30 pm
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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