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17th European White Dwarf Workshop: PROMPT - An effective tool for studies of pulsating stars
Barlow, Brad (2010)
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mla
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Barlow B. "17th European White Dwarf Workshop: PROMPT - An effective tool for studies of pulsating stars.", timms video, Universität Tübingen (2010): https://timms.uni-tuebingen.de:443/tp/UT_20100820_008_eurowd_0001. Accessed 30 Oct 2020.
apa
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Barlow, B. (2010). 17th European White Dwarf Workshop: PROMPT - An effective tool for studies of pulsating stars. timms video: Universität Tübingen. Retrieved October 30, 2020 from the World Wide Web https://timms.uni-tuebingen.de:443/tp/UT_20100820_008_eurowd_0001
harvard
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Barlow, B. (2010). 17th European White Dwarf Workshop: PROMPT - An effective tool for studies of pulsating stars [Online video]. 20 August. Available at: https://timms.uni-tuebingen.de:443/tp/UT_20100820_008_eurowd_0001 (Accessed: 30 October 2020).
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title: 17th European White Dwarf Workshop: PROMPT - An effective tool for studies of pulsating stars
alt. title: 17th European White Dwarf Workshop - Pulsating white dwarfs
creator: Barlow, Brad (author)
subjects: Astronomie, Physik, Astrophysik, Workshop, White Dwarf, PROMPT, pulsating stars, Brad Barlow
description: 17th European White Dwarf Workshop, 16. bis 20. August 2010
abstract: PROMPT - An effective tool for studies of pulsating stars (B.N. Barlow1, B.H. Dunlap1, J.C. Clemens1, D.E. Reichart2, K. Ivarsen2, A. LaCluyze2, J. Haislip2, M. Nysewander3) (1Department of Physics and Astronomy, University of North Carolina, Chapel Hill, NC 27599-3255, 2SKYNET, Department of Physics and Astronomy, University of North Carolina, Chapel Hill, NC 27599-3255, 3Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD, 21218) The Panchromatic Robotic Optical Monitoring and Polarimetry Telescopes (PROMPT) are a system of 0.41-m telescopes at CTIO in Chile built primarily for rapid and simultaneous multi-wavelength observations of gamma-ray burst afterglows. When not observing gamma-ray bursts, PROMPT is an indispensable tool for studies of pulsating stars. To illustrate its effectiveness, we present the O-C diagram for the sdBVr star CS 1246, including P-dot measurements and other intriguing results. The diagram was constructed from nearly 30,000 individual frames representing over 250 hours of time-series photometry.
publisher: ZDV Universität Tübingen
contributor: ZDV Universität Tübingen (producer)
creation date: 2010-08-20
dc type: image
localtype: video
identifier: UT_20100820_008_eurowd_0001
language: eng
rights: Url: https://timmsstatic.uni-tuebingen.de/jtimms/TimmsDisclaimer.html?637396151218459769