Columbia University 
Astronomy and Astrophysics


Jules P. Halpern

Teaching C3273: High-Energy Astrophysics

e-mail: jules@astro.columbia.edu

Telephone: (212) 854-2554


Research Interests:

Pulsars - I am investigating the extreme physical properties of neutron stars through timing and spectroscopy in X-rays and radio. This reveals their strongest magnetic fields, found in Anomalous X-ray Pulsars (AXPs), as well as their weakest, found in Central Compact Objects (CCOs). Monitoring the transient outbursts of AXPs is leading to an understanding of how their enormous magnetic field energy is converted to X-ray luminosity. In contrast, the relatively inconspicuous CCOs seem to have been born with very weak magnetic fields, and not much rotational energy either. This work makes use of the X-ray observatories Chandra, XMM-Newton, and Swift.

Gamma-ray Sources - The elusive unidentified high-energy gamma-ray sources originally discovered by the EGRET experiment on the Compton Gamma-Ray Observatory (CGRO) turn out to be pulsars and pulsar wind nebulae, supernova remnants, and maybe new classes as well. This subject has expanded into the very high-energy regime with the detection of TeV sources in the Galaxy by the ground-based Cerenkov telescopes H.E.S.S., MAGIC, Milagro. and VERITAS, and has literally "taken off" with the successful deployment of the Fermi Gamma-Ray Space Telescope. I will search for and study the counterparts of the gamma-ray sources at other wavelengths.

Background:

2000-present Professor, Department of Astronomy
1999-2005 Director, MDM Observatory
1994-2000 Associate Professor, Department of Astronomy
1992-1994 Research Scientist, Department of Astronomy
1989-1992 Associate Professor, Department of Physics
1984-1989 Assistant Professor, Department of Physics
1982-1984 Research Fellow in Astronomy, California Institute of Technology
1982 Ph. D., Harvard University
1976 S. B., Massachusetts Institute of Technology

Selected Publications:


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Last updated: January 21, 2010.