Calendar

Apr
24
Mon
Pizza Lunch: Laurel Farris
Apr 24 @ 12:30 pm – 1:30 pm
Pizza Lunch: Laurel Farris @ AY 119

Determining the size of coronal bright points using cross-correlation methods

Laurel Farris

 

Sep
1
Fri
Colloquium: Isak Wold (Host: Moire Prescott)
Sep 1 @ 3:15 pm – 4:15 pm
Colloquium: Isak Wold (Host: Moire Prescott) @ 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 a wide redshift range. To understand what types of galaxies are selected in LAE surveys – and how this evolves with redshift – it is important to establish a low-redshift reference sample that can be directly compared to high-redshift samples.  The lowest redshift where a direct Lya survey is currently possible is at a redshift of z~0.3 via the Galaxy Evolution Explorer (GALEX ) FUV grism data. Using the z~0.3 GALEX sample as an anchor point, it has been suggested that at low redshifts high equivalent width (EW) LAEs become less prevalent and that the amount of escaping Lya emission declines rapidly.  A number of explanations for these trends have been suggested including increasing dust content, increasing neutral column density, and/or increasing metallicity of star-forming galaxies at lower redshifts. However, the published z~0.3 GALEX sample is pre-selected from bright NUV objects.  Thus, objects with strong Lya emission but faint continuum (high-EW LAEs) could be missed.  In this talk, I will present my efforts to re-reduce the deepest archival GALEX FUV grism data and obtain a sample that is not biased against high-EW LAEs.  I will discuss the implications of this new sample on the evolutionary trends listed above.

Sep
20
Wed
Colloquium PhD Defense: Jean McKeever
Sep 20 @ 3:00 pm – 4:15 pm
Colloquium PhD Defense: Jean McKeever @ 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 its fundamental stellar properties with relative ease. There has been much exploration of solar-like oscillations within red giants with recent advances in technology, leading to new innovations in observing. The Kepler mission, with its 4-year observations of a single patch of sky, has opened the floodgates on asteroseismic studies. Binary star systems are also an invaluable tool for their ability to provide independent constraints on fundamental stellar parameters such as mass and radius. The asteroseismic scaling laws link observables in the light curves of stars to the physical parameters in the star, providing a unique tool to study large populations of stars quite easily. In this work we present our 4-year radial velocity observing program to provide accurate dynamical masses for 16 red giants in eclipsing binary systems. From this we find that asteroseismology overestimates the mass and radius of red giants by 15% and 5% respectively. We further attempt to model the pulsations of a few of these stars using stellar evolution and oscillation codes. The goal is to determine which masses are correct and if there is a physical cause for the discrepancy in asteroseismic masses. We find there are many challenges to modeling evolved stars such as red giants and we address a few of the major concerns. These systems are some of the best studied systems to date and further exploration of their asteroseismic mysteries is inevitable.

 

Jan
27
Mon
Pizza Lunch: Candace Gray
Jan 27 @ 12:30 pm – 1:30 pm
Pizza Lunch: Candace Gray @ AY 119

APO Open House Info

Candace Gray

Jan
29
Wed
ASTR 500 – Graduate Seminar
Jan 29 @ 12:00 pm – 1:00 pm
Jan
30
Thu
Astronomy on Tap
Jan 30 @ 7:00 pm – 9:30 pm
Astronomy on Tap @ Bosque Brewing Las Cruces Public House

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 Bosque Brewing website if you’re planning on attending!
https://www.bosquebrewing.com/bosque-brewing-events

Feb
5
Wed
ASTR 500 – Graduate Seminar
Feb 5 @ 12:00 pm – 1:00 pm
Feb
6
Thu
Colloquium: RESERVED
Feb 6 @ 3:15 pm – 4:15 pm
Colloquium: RESERVED @ BX102

Colloquium Title

Colloquium Speaker Name, Affiliation

Abstract text

Feb
10
Mon
Pizza lunch: Jon Holtzman
Feb 10 @ 12:30 pm – 1:30 pm
Pizza lunch: Jon Holtzman @ AY 119

pyvista: a data reduction framework

Jon Holtzman, NMSU

Feb
11
Tue
Remote Colloquium: RESERVED
Feb 11 @ 3:00 pm – 4:00 pm
Remote Colloquium: RESERVED @ MH 85

Colloquium Title

Colloquium Speaker Name, Affiliation

Abstract text