Anil Seth's
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Research

I am a postdoctoral fellow at the Harvard-Smithsonian Center for Astrophysics. For a list of publications go here (ADS), or click here for my Curriculum Vita.

My primary research interest is understanding the formation of nuclear star clusters and their relation to black holes. Nuclear star clusters are found at the centers of most galaxies and are the most massive and dense stellar collections in the universe.
I've worked on a number of projects related to nuclear star clusters:

  • Do Black Holes and Nuclear Star Clusters Co-exist? In a paper from 2008, we have shown that nuclear star clusters and black holes (as indicated by AGN) co-exist in all types of galaxies over a signficant range in mass.
  • How do Nuclear Star Clusters Form? Using observations of nearby edge-on spiral galaxies with HST, we found that these clusters are flattened in the plane of their host galaxy and have complex morphology and stellar populations, with younger disks of stars embedded in an older spheroid stars (basically self-similar to the larger galaxy structure!). These observations suggest that nuclear star clusters form from accretion of material (gas or star clusters) from their host galaxy disks.
  • What can we learn from the nearest nuclear star clusters? New adaptive optics technology allows us to study the kinematics of the nearest nuclear star clusters in great detail. Using a wide variety of telescopes, including adaptive optics corrected spectra from the Gemini telescope, I have embarked on a study of the nearest nuclear star. I've published the first of our targets last year which shows clear rotation. Detailed analysis of these observations combined with theoretical modeling will allow us to understand the details of the nuclear star cluster formation process and enable dynamical detection of any black holes within the nuclear star clusters.
I've also worked on a number of other projects studying galaxy evolution through stellar populations and stellar clusters in late-type (spiral and irregular) galaxies. These include:
  • For my PhD thesis, I analyzed the stellar populations of nearby edge-on galaxies with Julianne Dalcanton and Roelof de Jong. This work is published in two papers in the Astronomical Journal. Pretty pictures of the galaxies can be seen here.
  • I'm a part of two large Hubble Space Telescope projects focused on studying the resolved stars in nearby galaxies. The ANGST collaboration has used HST to image galaxies between 1-4 Mpc to determine their star formation histories. GHOSTS has focused on the stellar halos of nearby galaxies; studying the tenuous outer parts of galaxies can reveal their earliest history.

Personal

There to the left is my honey, Andrea, and myself enjoying ourselves on vacation in Santiago (photo credit to Marcel). For more pictures, check out my photo albums here.

You can email me at:
FIlastname@cfa.harvard.edu
where the 'FIlastname' above is aseth My personal email address is:
firstlast@gmail.com
Where the 'firstlast' is anilseth