low mass objects that cannot sustain Hydrogen fusion. I am interested in the
science that emereges from astrometric measurements of these substellar mass
objects. Since brown dwarfs can have masses from a few tenths the Sun's mass
down to a few Jupiter masses, studying them has implications on the two most
populous astronomical bodies in our solar neighborhood. Below is a description
of the BDKP, a program which encompasses the majority of my thesis.
Advisors: Mike Shara, AMNH, Fred Walter, Stony Brook, Adam Burgasser, MIT
The Brown Dwarf Kinematics Project (BDKP)OBJECTIVES:
within 20pc and a select sample of scientific interest
STATUS TO DATE:
PRIMARY SCIENTIFIC GOALS:
PRIMARY BDKP SCIENTISTS Jackie Faherty Adam Burgasser Kelle Cruz
IMPORTANT BDKP WEBSITES
Nstars A 2MASS based survey of stars and brown dwarfs within 20pc of the Sun
Dwarf Archives An archive of all confirmed L and T dwarfs
T Dwarf Archive An archive of all T dwarfs (may be out of date)
Spex Data for Dwarfs List of Spex prism for known 2MASS designation sources
Sloan L and T Archive An archive of all L and T dwarfs uncovered in Sloan
Very Low Mass Binaries Archive An archive of all stellar and substellar low mass binaries