Student Research Group
Summer Research 2013
Zack Li and Kelley Langhans, both rising sophomores, are working on different aspects of the problems of measuring and modeling the plasma temperature distribution in the shock-heated winds of massive stars.
New: The presentation I gave in January 2014 to recruit a student or two for my group provides a brief overview of my research and how students can contribute to it.
Summer Research 2012
Astrophysics major Jake Neely (2013) has been working on a project to analyze the X-ray line emission in the O stars ζ Ori and ζ Pup, as measured with the Reflection Grating Spectrometer on the XMM X-ray Telescope. Jake is using these data to derive elemental abundances in these massive stars winds, and address questions related to rotational mixing and chemical evolution in O stars.
Summer Research 2011
Sierra Eckert ('14) and Jackson Goodman ('13) have started working on projects involving X-ray emission line profiles in massive stars. Neither of them were on campus this summer, but they're continuing their projects in the fall.
Summer Research 2010
Tzitlaly Barajas (Cal. State Los Angeles, '12) worked with the Peter van de Kamp Observatory here on campus to study Bp and other magnetic massive stars. While James MacArthur ('11) worked on a new project: using the curve of growth technique to measure the column density and ionization balance in X-ray photoionized neon plasma we're studying at the Z-Machine facility at Sandia National Lab.
To get a sense of other student projects that my student-based research group will be working on in the future, you can check out this brief presentation about potential projects I gave in February 2009. The project on the laboratory astrophysics experiments and modeling is described in the poster by my old student, Michael Rosenberg, who did some preliminary work on the project two summers ago.
Summer Research 2009
James MacArthur ('11), a physics major, worked with some new Chandra observations this summer, with his project continuing into the semester. He presented his preliminary research results at the American Astronomical Society meeting in January (see below). We're working - along with Marc Gagné at West Chester and Leisa Townsley at Penn State - on trying to understand the strong X-ray emission from a pair of binary stars in M17.
Jan. 2010: James MacArthur has presented his preliminary research results at the American Astronomical Society meeting in Washington, DC, with a poster entitled, "The Source of Anomalously Hard X-rays in M17's Central O4-O4 Binary".
Aug. 2011: James helped out on another project, using his expertise with spectroscopy in crowded Chandra fields. He's a coauthor on our group's study of HD 93129A, one of the most massive stars in the Galaxy.
Vernon Chaplin ('07) has published a paper: "Spectroscopic Measurements of Temperature and Plasma Impurity Concentration During Magnetic Reconnection at the Swarthmore Spheromak Experiment," in Physics of Plasmas that was based on his senior thesis at Swarthmore. Congratulations, Vernon!
Erin Martell and Emma Wollman presented a poster about their stellar wind research at the Atomic Processes in Plasmas meeting in Monterey, California in March 2009. They won the prize for the best student poster at the meeting.
July 2010: Emma's work on the X-ray line profiles of the massive star, zeta Puppis, has been published.
Aug. 2010: Erin's work on the broad-band X-ray spectral trends among massive stars has been published.
2009: Emma Wollman ('09) studied Greek, and modeled the resolved X-ray line profiles in the Chandra spectra of several massive stars. Erin Martell ('09) studied Latin, and analyzed the morphological trends in the Chandra spectra of over a dozen massive stars.
Emma gave a presentation at the 19th Annual Keck Northeast Astronomy Consortium Student Research Symposium, at Wesleyan University in November 2008, titled, "Spectral Modeling of X-rays from Hot Star Winds." You can look at her talk and read her paper.
Upon graduation, both Erin and Emma received High Honors in their external honors examinations. Erin won the Department's Berman Prize. Emma won the Department's Elmore Prize as well as the College's Lang Award. Erin is now attending the University of Chicago's astronomy and astrophysics program (update: Erin has won a Clare Boothe Luce Fellowship), while Emma is in Caltech's physics program (working with Keith Schwab's research group).
2008:Mike Rosenberg ('08) was a physics major, and entered the Physics PhD program at MIT, continuing his study of plasma physics, after graduating. His research project involved modeling the x-ray photoionization of plasma at the Z-Machine, with applications to astrophysics. This was the basis of Mike's senior honors thesis. In September 2007, Mike presented some preliminary results of his thesis research at the Swarthmore student research poster session, sponsored by Sigma Xi [ppt, png, pdf].
Older graduates include Vernon Chaplin ('07), Mike Kuhn ('07), Steve St. Vincent ('07), Victoria Swisher ('06), Micah Walter-Range ('06), Kevin Grizzard (St. John's College '06), Casey Reed ('05), Nate Shupe ('05), Marty Mudd (Williams '04), Mark Janoff ('04), Rachel Sapiro ('04), Eric Levy ('04), Kate Penrose ('04), Dave Conners ('03), Elliot Reed ('03), Carie Cardamone (Wellesley '02), Stephanie Tonnesen ('03), Roban Kramer ('03), and Allison Adelman (Bryn Mawr '03).After leaving Swarthmore, these people have done things like worked in Vietnam, worked on science policy at the National Academy of Sciences, gone to law school, to graduate school in international relations, linguistics, physics, and astrophysics, and become a science librarian at a small liberal arts college.
Students who wrote honors theses under David's direction include:
Some of our work is supported through Prism Computational Sciences, in Madison, Wisconsin. Prism is a small company that does basic and applied physics research and code development. It is run by Dr. Joe MacFarlane, who is a long-time collaborator of ours.
Mike Rosenberg used the VisRad view-factor code, from Prism Computational Sciences, to make an animation of the imploding Z-pinch wire array at the Z-Machine facility at Sandia, as part of his senior thesis work.
You can also access information about older students and their presentations.
Astrobetter - lots of useful information about the nitty-gritty of astronomical research
Student Travel and Research Funding
HHMI travel funding
Grad School Information
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|David Cohen: cohen -at- astro -dot- swarthmore -dot- edu
Last modified: January 29, 2014