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Joseph Wellhouse

Research/Teaching Assistant
Entered: 2005
Office: 220 Astronomy
Phone: (575)646-8180
Fax: (575)646-1602
 
E-mail: jwell
(append "@nmsu.edu")
 
Photo
B.S. Harvey Mudd College, 2005

Research

I started my graduate work in fall 2005, working with Dr. Tom Harrison. My principal interests are in CVs, star formation, and stellar evolution.

My present work is focused on understanding the accretion disk and secondary star around the cataclysmic variable WZ Sagittae. In particular, molecules have been identified in IR spectra and we hope to identify their origin.

Concerning another project, recent work has suggested that the accepted evolutionary track for cataclysmic variables, CVs, may be in error. Measurements of carbon abundances have suggested that the secondary stars in these systems may have undergone far more changes during the formation of the CV than previously thought. Magnetic and non-magnetic CVs also appear to follow different evolutionary tracks. A principal probe of this evolution is metal abundance in the secondary star.

To expand our understanding in this area, we have obtained near infrared spectra of a sample of CVs with SPEX on the NASA Infrared Telescope Facility. These data permit quantitative measurements of carbon and other metal abundances in the secondary stars with the aid of a stellar atmosphere model. We have used the program SPECTRUM to generate these models. We find that both AE Aqr and GK Per show extreme carbon 12 deficits. In the future we plan to extend these models to include Na, Mg, and Fe.

I have previously worked with infrared observations, studying dust extinction in star clusters from data taken with the 1-meter telescope at the Table Mountain Observatory and the Two Micron All Sky Survey. I have also worked at the Spitzer Science Center, analyzing Chandra x-ray data for several binary systems to probe for their infrared counterparts, and also used the 2MASS survey data to study infrared counterparts of white dwarfs. My senior thesis project at HMC focused further on these objects, to understand the properties of magnetic white dwarfs and identify possible white dwarf + low mass Main Sequence pairs.

Meetings

January 2007: American Astronomical Society meeting, Near Infrared Quantitative Abundance Analysis of The Secondary Stars in a Sample of CVs
J.W. Wellhouse & T.E. Harrison

January 2007: American Astronomical Society meeting, Cool Companions of White Dwarfs from 2MASS
D W. Hoard, S. Wachter, L. K. Sturch, A. M. Widhalm, K. P. Weiler, J. W. Wellhouse, & M. Gibiansky

January 2006: American Astronomical Society meeting, The Origin of the Molecular Emission in WZ Sagittae
J.W. Wellhouse, T.E. Harrison, S.B. Howell, & P. Szkody

January 2005: American Astronomical Society meeting, Magnetic White Dwarfs in the Infrared
J. W. Wellhouse, D. W. Hoard, S. B. Howell, & S. Wachter

Publications

Magnetic White Dwarfs in the Two Micron All Sky Survey: A Search for Candidate Binary Systems
J. W. Wellhouse, D. W. Hoard, S. B. Howell, S. Wachter, & A. A. Esin 2005, PASP, 117, 1378

Chandra HRC Localization of the Low-Mass X-Ray Binaries X1624-490 and X1702-429: The Infrared Counterparts,
S. Wachter, J. W. Wellhouse, S. K. Patel, A. P. Smale, J. F. Alves, & P. Bouchet 2005, ApJ, 621, 393

My CV in PDF format.




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