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Uma P. Vijh

Researcher at University of Toledo

Publications -  46
Citations -  3236

Uma P. Vijh is an academic researcher from University of Toledo. The author has contributed to research in topics: Large Magellanic Cloud & Galaxy. The author has an hindex of 27, co-authored 46 publications receiving 3095 citations. Previous affiliations of Uma P. Vijh include National Science Foundation & Association of Universities for Research in Astronomy.

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Surveying the Agents of Galaxy Evolution in the Tidally Stripped, Low Metallicity Small Magellanic Cloud (SAGE-SMC). I. Overview

Karl D. Gordon, +63 more
TL;DR: In this paper, the SAGE-SMC (Surveying the Agents of Galaxy Evolution in the Tidally stripped, low metallicity Small Magellanic Cloud) Spitzer Legacy program was used to study the amount and type of dust in the present interstellar medium.
Journal ArticleDOI

Surveying the Agents of Galaxy Evolution in the Tidally-Stripped, Low Metallicity Small Magellanic Cloud (SAGE-SMC). I. Overview

TL;DR: In this paper, the SAGE-SMC (Surveying the Agents of Galaxy Evolution in the Tidally stripped, low metallicity Small Magellanic Cloud) Spitzer Legacy program with the specific goals of studying the amount and type of dust in the present interstellar medium, the sources of dust of evolved stars, and how much dust is consumed in star formation.
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Spitzer SAGE Survey of the Large Magellanic Cloud. II. Evolved Stars and Infrared Color-Magnitude Diagrams

TL;DR: In this article, color-magnitude diagrams (CMDs) are presented for the Spitzer SAGE (Surveying the Agents of a Galaxy's Evolution) survey of the Large Magellanic Cloud (LMC).
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The SAGE-Spec Spitzer Legacy programme: the life-cycle of dust and gas in the Large Magellanic Cloud - Point source classification I

Paul M. Woods, +62 more
TL;DR: In this article, a decision-tree method of object classification based on infrared spectral features, continuum and spectral energy distribution shape, bolometric luminosity, cluster membership and variability information was used to classify the SAGE-Spec sample of point sources.