RESEARCH INTERESTSStar formation, stellar evolution, environmental effects on star and planet formation, the initial mass function and primordial stellar binarity.The physics of ultracool dwarfs: their formation, atmospheres and evolution.
CURRENT RESEARCHI have recently completed work on the nearby binary brown dwarfs Indi Ba and Bb. I reduced VLT photometry and spectroscopy from the optical through to the thermal-IR (0.6-5.1 micron) which allowed a detailed comparison with atmospheric and evolutionary models of sub-stellar objects at intermediate age. The comparison with the Lyon atmospheric models has identified areas of the models where improvements can be made and also highlighted the problem of deriving inaccurate physical properties even for seemingly well-constrained systems. I am also involved in the astrometric monitoring of this binary which has allowed a preliminary determination of the total system mass and on-going absolute astrometry will determine the mass ratio and hence the individual masses. Together with the luminosity determinations, these observations will provide an extremely well characterised system which will tightly constrain future evolutionary models. I am now using optical and near-IR observations along with Chandra X-ray observations to determine characteristics of stars in young stellar clusters. We hope to combine these multi-wavelength data for 10-20 clusters in massive star-forming environments, to consistently compare properties such as evidence of mass segregation, binarity and the form of the IMF, free of the problems associated with a myriad of selection techniques. I am also using high-resolution spectroscopy of nearby FGK stars in an attempt to identify young stellar targets for follow-up planet searches with the next generation of high-constrast imagers Finally, I am searching for and characterising substellar companions to young stars involving the characterisation of ~12 young L dwarfs by comparison of their near-IR spectra to synthetic stellar spectra. The existing measurments of these objects are being extended into the thermal-IR regime which will allow us to more accurately determine their luminosities and effective temperatures as well as allowing a probe of the L to T transition in young objects.
EMPLOYMENTUniversity of Exeter, Exeter, Devon, UKOct. 2009-present
EDUCATIONUniversity of Exeter, Exeter, Devon, UK2005-2009
University of St Andrews, St Andrews, Fife, UK
Clyde Valley High School, Overtown, North Lanarkshire, UK
PUBLICATIONS
Indi Ba, Bb: a detailed study of the nearest known
brown dwarfs
The UKIDSS-2MASS Proper Motion Survey I: Ultracool dwarfs from UKIDSS DR4
The UV-Excess survey of the Northern Galactic Plane (UVEX)
The highest resolution near-IR spectrum of the imaged planetary mass companion 2M1207b
The Effect of Stellar Density of Star-Forming Regions on Stellar Multiplicity (in prep.)
A Compendium of Near-IR Spectra of Young, Very Low-Mass Companions (in prep.)
Star formation and disk properties in Pismis 24 (in prep.)
Dynamical System Mass of Indi Ba, Bb: the relative orbit (in prep.)
Individual Dynamical Masses of Indi Ba and Bb: the absolute orbit (in prep.)
Infrared properties of the X-ray emitting young stellar objects in the Carina Nebula
(in prep.)
An Introduction to the Chandra Carina Complex Project (in prep.)
A Catalog of Chandra X-ray Sources in the Carina Nebula (in prep.)
A Chandra ACIS Study of the Young Open Cluster Trumpler 15 in Carina (in prep.)
Trumpler 16 as Viewed by the Chandra Carina Complex Project (in prep.)
X-ray Star Clusters in the Carina Complex (in prep.)
CONFERENCE PROCEEDINGS
Indi Ba, Bb: a spectroscopic study of the nearest known brown dwarfs
Dynamical masses of the nearest brown dwarf binary: Indi Ba, Bb
TELESCOPE PROPOSALSI am P.I. on an ESO proposal entitled Characterising the IMF of two high-mass star-forming regions with the VLT and Chandra and a follow-up proposal Characterising the IMF in a range of high-mass star-forming regions with the VLT and Chandra which will allow us to investigate the IMF in different high-mass environments.I am a co-investigator on a series of proposals to determine astrometrically, the dynamical system mass and individual masses of the nearest brown dwarf binary, Indi Ba, Bb (McCaughrean P.I.). I am also a co-investigator on a HAWK-I science verification proposal The Carina Nebula as a laboratory of massive star feedback (Preibisch P.I.) and on an NSF proposal The origins and environments of rich young stellar clusters (Feigelson P.I.) I have also recently made use of the 2m robotic Liverpool Telescope for photometric and spectroscopic observations.
OBSERVING EXPERIENCE
Southern Astrophysical Research Telescope January 2011
TEACHING EXPERIENCEUniversity of Exeter
University of St Andrews
COMPUTING SKILLS
REFEREES
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