NMSUAstronomy

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Research » Stellar, Helioseismology, and Exoplanetary Group


The stellar group at NMSU is active in research on interacting binaries (particularly cataclysmic variables and binary black holes), stellar dynamics such as those in globular clusters, variable stars, and helioseismology. Researchers make use of the facilities at Apache Point Observatory and have obtained time on the Keck telescopes, Gemini, and NOAO telescopes in both Arizona and Chile. Continuing research projects also include using the Hubble Space Telescope to obtain parallaxes of both cataclysmic variables and galactic Cepheid variables in order to obtain accurate distances to these objects. You can find more details about our various research projects here.


Killer Stars

Associations

New Stars

Star Clusters

Sun

Seismology

Particular interests of members include the following.

Thomas Harrison  Observatory Research Specialist
Cataclysmic variables; infrared spectroscopy
 
Jason Jackiewicz  Assistant Professor
Helioseismology
 
Joni Johnson Research Fellow
Cataclysmic variables; PAGB stars
 
Bernie McNamara  Professor
Stellar dynamics, X-ray variable stars; gamma-ray bursts
 
Jillian Bornak    Graduate Student
Stellar remnants; accretion processes; X-ray binaries
 
Mary Jo Clark Graduate Student
Massive star evolution; gamma-ray bursters; high-energy astrophysics
 
Jeff Coughlin Graduate Student
Extrasolar planets; eclipsing binaries; stellar populations
 
Ryan Hamilton Graduate Student
Stellar populations
 
Michael Kirk Graduate Student
Solar astronomy