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Hillenbrand's astronomical research is in the area of star and planet formation, specifically regarding processes associated with the formation and early evolution of young stellar objects. Her observational and data analysis experience covers wavelengths from x-ray to millimeter, though focusing mostly on optical/near-infrared science. The most well-known research accomplishments include evidence for circumstellar (protoplanetary) disks associated with Herbig Ae/Be stars, determination of the stellar and sub-stellar initial mass function in the Orion Nebula Cluster, studies of age spreads in star forming regions, determination of evolutionary timescales for circumstellar dust in both primordial and debris disks, and episodic accretion in young stellar objects. Other research interests include star clusters, stellar angular momentum evolution, stellar age indicators, protostars, accretion and accretion-driven wind phenomena, young planets, variability phenomena in young stars, stellar multiplicity. Hillenbrand has over 300 refereed publications, 25 as first author.
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The Astrophysical Journalno. 2 (2023): 102-102
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L. M. Rebull, J. R. Stauffer, J. Bouvier,Ann Marie Cody,Lynne A. Hillenbrand,David R. Soderblom,Jeff A. Valenti, D. Barrado, H. Bouy,David R. Ciardi,Marc H. Pinsonneault,Keivan G. Stassun,
arxiv(2016)
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