Columbia Astrophysics Laboratory
Arlin Crotts
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Teaching, Autumn 2009 Course: C1403 "Earth, Moon & Planets"
Research Interests:
- The nature of quasar absorption lines and the intergalactic medium
- Galaxy formation, galactic haloes: gravitational microlensing in M31
- Star formation, the interstellar medium in the Large Magellanic Cloud: light echoes from SN 1987A
- Understanding lunar outgassing and optical
transients
I am interested in how matter on cosmological and galactic scales has
rearranged itself over the life of the Universe. Our studies of Lyman alpha
forest absorbers in the spectra of quasars, for example, showed that at early
times a large fraction of the baryonic matter in the Universe was tied up in
these clouds, which we showed to be much larger in diameter than previously
suspected. We have embarked on a number of projects to determine better how
these objects evolve in size, what their shape is, and how they fit into large
scale structure at different stages of the Universe. We are also studying
whether the objects that compose the dark matter in M31 fall within the mass
range (slightly less massive than the Sun) seen by gravitational microlensing
studies of our Galaxy's halo. A study of M31's halo microlensing promises to
better establish the spatial distribution of these objects, and perhaps their
component mass distribution, while being sensitive to halo masses as small as
10-8M
. We have also taken the unique opportunity of the explosion of
Supernova 1987A in the vicinity of the 30 Doradus star-forming region in the
nearby galaxy, the Large Magellanic Cloud, to follow the reflection of the
supernova light (or "light echo") from surrounding material in the manner of a
radar pulse, using it to map the structure in three dimensions of the
interstellar medium affected by star formation processes, as well as the
supernova's circumstellar material, which was affected by the late stages of
evolution of the star that exploded. Soon this structure will brighten once
more as Supernova Remnant 1987A, as the debris from the explosion strikes the
surrounding material that we have mapped.
In addition to my research into astronomical and cosmological systems, I also build astronomical instrumentation, most recently the MDM 8K, a 67 million pixel CCD imager which has become one of the most popular instruments at MDM Observatory. I am also building and designing instrumentation connected with large aperture, liquid mirror telescopes, most notably the LZT, ALPACA and LLAMA projects.
Background:
| 2004 - present | Professor, Department of Astronomy, Columbia University |
| 1996 - 2004 | Associate Professor, Department of Astronomy, Columbia University |
| 1991 - 1996 | Assistant Professor, Department of Astronomy, Columbia University |
| 1988 - 1990 | Nat'l Research Council Associate, NASA Goddard Space Flight Center |
| 1985 - 1988 | McDonald Postdoctoral Fellow, The University of Texas at Austin |
| 1986 | Ph.D., The University of Chicago (Physics) | 1980 | A.B., Princeton University (Physics) |
Selected Publications:
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