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Elizabeth A. Lada

Researcher at University of Florida

Publications -  104
Citations -  12218

Elizabeth A. Lada is an academic researcher from University of Florida. The author has contributed to research in topics: Star formation & Molecular cloud. The author has an hindex of 43, co-authored 104 publications receiving 11648 citations. Previous affiliations of Elizabeth A. Lada include National Science Foundation & Association of Universities for Research in Astronomy.

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Journal ArticleDOI

Embedded Clusters in Molecular Clouds

TL;DR: The first extensive catalog of galactic embedded clusters is compiled, finding that the embedded cluster birthrate exceeds that of visible open clusters by an order of magnitude or more indicating a high infant mortality rate for protocluster systems.
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Disk Frequencies and Lifetimes in Young Clusters

TL;DR: In this paper, the authors report the results of the first sensitive L-band survey of the intermediate-age (2.5-30 Myr) clusters NGC 2264, NGC 2362, and NGC 1960.
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A Census of the Young Cluster IC 348

TL;DR: In this paper, a new census of the stellar and substellar members of the young cluster IC 348 is presented, which contains a total of 288 members, 23 of which are later than M6 and thus are likely to be brown dwarfs.
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Internal structure of a cold dark molecular cloud inferred from the extinction of background starlight.

TL;DR: Sensitive near-infrared measurements of the light from background stars as it is absorbed and scattered by trace amounts of dust are used to probe the internal structure of the dark cloud Barnard 68 with unprecedented detail and find the cloud's density structure to be very well described by the equations for a pressure-confined, self-gravitating isothermal sphere that is critically stable according to the Bonnor–Ebert criteria.
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Dust Extinction and Molecular Gas in the Dark Cloud IC 5146

TL;DR: In this article, a method for mapping the distribution of dust through a molecular cloud using data obtained in large-scale, multi-wavelength, infrared imaging surveys is described, which combines direct measurements of near-infrared color excess and certain techniques of star counting to derive mean extinctions and map the dust column density distribution through a cloud at higher angular resolutions and greater optical depths.