N
Nathan Smith
Researcher at University of Arizona
Publications - 543
Citations - 30830
Nathan Smith is an academic researcher from University of Arizona. The author has contributed to research in topics: Supernova & Nebula. The author has an hindex of 86, co-authored 503 publications receiving 28124 citations. Previous affiliations of Nathan Smith include University of Hawaii at Manoa & University of California.
Papers
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SN2012ab: A peculiar Type IIn supernova with aspherical circumstellar material
Christopher Bilinski,Nathan Smith,G. Grant Williams,Paul S. Smith,Wei Kang Zheng,Melissa L. Graham,Jon C. Mauerhan,Jennifer E. Andrews,Alexei V. Filippenko,Carl W. Akerlof,Emmanouil Chatzopoulos,Jennifer L. Hoffman,Leah Huk,Douglas C. Leonard,George H Marion,Peter Milne,Robert M. Quimby,Jeffrey M. Silverman,Jozsef Vinko,Jozsef Vinko,Jozsef Vinko,J. Craig Wheeler,Fang Yuan,Fang Yuan +23 more
TL;DR: In this paper, Bengier et al. presented the results of a postdoctoral fellowship at the University of New South Wales (UNSW) with the NSF Astronomy and Astrophysics Postdoctoral Fellowship.
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SIMBA Observations of the Keyhole Nebula
TL;DR: In this paper, the SIMBA bolometer at SEST was used to measure the 1.2 mm continuum emission toward the keyhole nebula, which is attributed to thermal free-free emission.
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Extended red objects and stellar-wind bow shocks in the Carina Nebula
Remington O. Sexton,Remington O. Sexton,Matthew S. Povich,Nathan Smith,Brian Babler,Marilyn R. Meade,Alexander L. Rudolph +6 more
TL;DR: In this paper, the results of infrared photometry on 39 extended red objects (EROs) in the Carina Nebula, observed with the Spitzer Space Telescope, were reported.
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[TiII] and [NiII] emission from the strontium filament of eta Carinae
TL;DR: In this article, the authors studied the nature of the [TiII] and [NiII] emission from strontium filament found in the ejecta of eta Carinae.
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Massive star formation and feedback in W49A: the source of our Galaxy's most luminous water maser outflow★
TL;DR: In this article, the authors locate the source of the water maser outflow at the position of the compact mid-IR peak of source G (source G:IRS1) to within 0.