Calendar

Mar 20 @ 3:15 pm – 4:15 pm BX102
Colloquium Title Colloquium Speaker Name, Affiliation Abstract textShare this:TweetPrint
Apr 3 @ 3:15 pm – 4:15 pm Online
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 Online
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 20 @ 9:00 am – 10:00 am Online
The role if the intergalactic medium in the baryon cycle Valentina D’Odorico, INAF Osservatorio Astronomico di Trieste The intergalactic medium (IGM) plays a relevant role in galaxy evolution being the reservoir of gas for star...
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Apr 24 @ 9:00 am – 10:00 am Remote
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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Apr 27 @ 12:30 pm – 1:30 pm Online
Competing effects of the duty cycle and scatter around star formation during reionization as observed by JWST and SKA Sultan Hassan, NMSUShare this:TweetPrint
May 4 @ 12:30 pm – 1:30 pm Online
ASTR 598 Kelly Sanderson, NMSUShare this:TweetPrint
May 8 @ 3:00 pm – 4:00 pm Remote via Zoom
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 15 @ 3:15 pm – 4:15 pm BX102
Colloquium Title Colloquium Speaker Name, Affiliation Abstract textShare this:TweetPrint
May 29 @ 2:30 pm – 3:30 pm Online
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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