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17th European White Dwarf Workshop: Latest Results From The DODO Survey - Imaging Planets Around White Dwarfs
Hogan, Emma (2010)
clipboard
mla
clipboard		 Hogan E. "17th European White Dwarf Workshop: Latest Results From The DODO Survey - Imaging Planets Around White Dwarfs.", timms video, Universität Tübingen (2010): https://timms.uni-tuebingen.de:443/tp/UT_20100819_018_eurowd_0001. Accessed 25 Apr 2024.
apa
clipboard		 Hogan, E. (2010). 17th European White Dwarf Workshop: Latest Results From The DODO Survey - Imaging Planets Around White Dwarfs. timms video: Universität Tübingen. Retrieved April 25, 2024 from the World Wide Web https://timms.uni-tuebingen.de:443/tp/UT_20100819_018_eurowd_0001
harvard
clipboard		 Hogan, E. (2010). 17th European White Dwarf Workshop: Latest Results From The DODO Survey - Imaging Planets Around White Dwarfs [Online video]. 19 August. Available at: https://timms.uni-tuebingen.de:443/tp/UT_20100819_018_eurowd_0001 (Accessed: 25 April 2024).
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Information
title: 17th European White Dwarf Workshop: Latest Results From The DODO Survey - Imaging Planets Around White Dwarfs
alt. title: 17th European White Dwarf Workshop - Disks, dust and planets around white dwarfs
creator: Hogan, Emma (author)
subjects: Astronomie, Physik, Astrophysik, Workshop, White Dwarf, DODO Survey, Imaging Planets Around White Dwarfs, Emma Hogan
description: 17th European White Dwarf Workshop, 16. bis 20. August 2010
abstract: Latest Results From The DODO Survey: Imaging Planets Around White Dwarfs (Emma Hogan, Matt Burleigh, Fraser Clarke) (Gemini Observatory, University of Leicester, University of Oxford) The aim of the Degenerate Objects around Degenerate Objects (DODO) survey is to search for very low mass brown dwarfs and extrasolar planets in wide orbits around white dwarfs via direct imaging. The detection of a planet around a white dwarf would prove that such objects can survive the final stages of stellar evolution and place constraints on the frequency of planetary systems around their progenitors (with masses between 1.5 - 8 solar masses, i.e., early B to mid F). This talk presents the latest results of our multi-epoch J band common proper motion survey of nearby equatorial and northern hemisphere white dwarfs.
publisher: ZDV Universität Tübingen
contributor: ZDV Universität Tübingen (producer)
creation date: 2010-08-19
dc type: image
localtype: video
identifier: UT_20100819_018_eurowd_0001
language: eng
rights: Url: https://timmsstatic.uni-tuebingen.de/jtimms/TimmsDisclaimer.html?638496036276011490