Research Assistant Professor
Five College Radio Astronomy
Observatory
University of Massachusetts,
Amherst 01003.
Phone: (413) 545 0925;
Fax: (413) 545 4223
Email: gopal@fcrao1.astro.umass.edu
Ph.D., Astronomy, 1997, University of Arizona.
M.S. Electrical Engineering, 1990, Caltech.
B.E. Electronics & Communication Engineering, 1989, Anna University,
Madras, India.
Curriculum Vitae [ html format] [ pdf format]
List of Publications
Research
Radio Astronomy, Molecular clouds and star formation. Development of advanced
mm and sub-mm receivers.
Motivation: One of the major goals of modern-day observational astronomy is the
identification and study of protostellar objects. A study of
protostars will provide knowledge of the physics and initial
conditions required for star formation, protostellar evolution, and
the formation of solar systems like our own. In the earliest phases of
star formation, protostellar objects are highly obscured in a cocoon
of dust and gas, and hence, are not observable with optical or infrared
telescopes. While continuum observations at longer wavelengths can
help identify protostellar candidates, spectroscopy is required to
understand the underlying kinematics in protostellar regions. Because
of the large obscuration and cold temperatures found in protostellar
cores, there is an abundance of molecular species in young stellar
objects (YSOs).
Thus, millimeter (mm) and submillimeter (submm) molecular line
observations provide the best opportunities to study the morphology,
chemical composition and dynamics of YSOs. Low noise, heterodyne
receivers at mm and submm wavelengths are the instruments of choice
for observation of star-forming regions, because of their high
sensitivities and spectral resolution. Therefore, many of the
mysteries surrounding the star formation process can be solved by
observations with sensitive mm and submm heterodyne receivers, and
careful analysis of the results.
Approach: I am tackling the problem of star formation using a a multi-pronged
approach. Towards this end, I am involved in the following major
activities. Please follow the respective links for more details.
- Instrumentation
- Development of advanced mm and submm receivers and subsystems
- Theoretical Modeling
- Theoretical radiative transfer modeling of the emergent spectra from
star-forming regions.
- Observations
- A vigorous observational program at mm
and submm wavelengths with the purpose of identifying and studying
protostellar objects.
Working with Mark
Heyer and Mike
Brewer, I have ported the FCRAO data analysis package, SPA to
linux. If you are an FCRAO observer and use the linux operating
system, you can download the
debian .deb package or the
redhat rpm package for SPA. You will need xgterm from the x11iraf software
package. x11iraf is available as a debian
package. A
user manual for SPA is also available. If you are not an FCRAO
observer, you obviously do not need this package.
I have also written a new
Gildas language called (unimaginatively) FCRAO that
converts FCRAO SPA data directly to the CLASS data
format. For now, FCRAO is only available for linux. You can
download the debian package
or the redhat package
for v1.1 of fcrao.
Other Astronomy Software Links:
Debian is currently the most popular "non-commercial" version of the
Linux operating system. The keys
to Debian's success are its unique social contract, and
ongoing development by over 500 volunteer
developers
worldwide who maintain more than 2500 free software packages,
collaborating over the internet. I am proud to be an official debian
developer. I maintain a few packages, some of which are related to
astronomy. Another cool feature of Debian linux is it's Bug Tracking
System (BTS). You can find out how conscientious I am in dealing with
bugs in my packages by checking
my BTS entries.
- Chris Devries'
home page. I'm guiding his PhD. thesis.
- Steward Observatory Radio Astronomy Laboratory (SORAL) - I still collaborate with them.
- Some observatory links:
Last modified: Sept. 21, 2000.
gopal@astro.umass.edu