PPT-Mapping the HI Neighborhood Around Starburst Dwarf Galaxies

Author : giovanna-bartolotta | Published Date : 2016-10-31

Megan Johnson NRAO Green Bank TullyFisher Workshop April 2012 Outline Introduction NGC 1569 Review of stellar and gas kinematics from LITTLE THINGS GBT map NGC

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Mapping the HI Neighborhood Around Starburst Dwarf Galaxies: Transcript

Megan Johnson NRAO Green Bank TullyFisher Workshop April 2012 Outline Introduction NGC 1569 Review of stellar and gas kinematics from LITTLE THINGS GBT map NGC 4163NGC 4214 Future Work. Adam Leroy. National Radio Astronomy Observatory. HERITAGE (. Meixner. et al.). Dust in Dwarf Galaxies. Adam Leroy. National Radio Astronomy Observatory. HERITAGE (. Meixner. et al.). SAGE (. Meixner. as Seen at . Very High Energies. Elisa Prandini . Dipartimento. . di. . Fisica. & INFN Padova. . prandini@pd.infn.it. Dipartimento. . di. . Astronomia. , . Padova, 23. rd. June 2011. Outline. Rich Dwarf Galaxies. . Sambit. . Roychowdhury. (NCRA), . Jayaram. . N. . Chengalur. . (. NCRA. ), . . Igor . D. . Karachentsev. (SAO. ), Margarita . Sharina. (SAO). Ayesha Begum . 5-1013 MSun Diameter: 1-200 kpc Luminosity: 106-1012 little or no rotation, so we can 12 Oct 2012. Banyuls. MODELING COUNTS AND CIBA WITH MAIN SEQUENCE AND STARBURST GALAXIES. Matthieu. Béthermin. CEA . Saclay. In collaboration with Mark Sargent, . Emanuele. . Daddi. , . Georgios. . Giuseppina. . Battaglia. Instituto. de . Astrofisica. de Canarias, Tenerife. Credit. : ESO/. H.H.Heyer. Credit. : ESO/L. . Calçada. Karachentsev. et al. 2014. Individual . Red . Giant Branch . stars. metallicity. star-forming dwarf galaxies. Diane Cormier . ITA, ZAH, University of Heidelberg – group of Frank . Bigiel. Suzanne Madden, . Vianney. . Lebouteiller. , . Sacha. . Hony. , Fr. é. d. Dwarf Galaxies in . Fornax. . Shed . Light on a Cosmological Mystery. National Science Foundation • Division of Astronomical Sciences . Prepared by the . Association of Universities for Research in Astronomy . Kaiki Taro Inoue . (KINDAI U.). Seminar. @Osaka U 22 Feb 2017. Outline. Missing Satellite Problem. Gravitational Lensing . Substructure vs Line-of-sight Halos. ALMA Observations (SDP.81, MG0414+0534). Universe. Imagine that you find a star with an unknown distance, but you notice that it has a distinctive characteristic that tells you that it is a specific type of star. And let’s imagine that all stars of that type have the same luminosity, and you happen to know the value of that luminosity. You can then estimate the distance for the star you found from the inverse square law of light:. Astronomy C Event 2019. Stellar Evolution in Normal & Starburst Galaxies. Supported by NASA’s Universe of Learning STEM Network. . NASA’s Universe of Learning Network/CXC/NSO . Stephen Hawking - The Birth of Stars - YouTube. Life Cycle of Stars. Nebula – large cloud of gas and dust spread out in an immense volume. Life Cycle of Stars. Gravity pulls gas and dust together in the densest part of the nebula. stellar core remnant. composed mostly of . electron-degenerate matter. . A white dwarf is very . dense. : its mass is comparable to the . Sun. 's, while its volume is comparable to the . Earth. 's. A white dwarf's faint . How Galaxies form Stars – August 24 2016 . Robbert. Verbeke. 1. Bert . Vandenbroucke. Sven De . Rijcke. Ghent University. 1. Robbert.verbeke@ugent.be. @. Rbhfd. Λ. CDM. Standard model for cosmology.

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