PPT-Simulations of realistic dwarf galaxies including Pop III feedback

Author : jacey | Published Date : 2024-02-16

How Galaxies form Stars August 24 2016 Robbert Verbeke 1 Bert Vandenbroucke Sven De Rijcke Ghent University 1 Robbertverbekeugentbe Rbhfd Λ CDM Standard model

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Simulations of realistic dwarf galaxies including Pop III feedback: Transcript

How Galaxies form Stars August 24 2016 Robbert Verbeke 1 Bert Vandenbroucke Sven De Rijcke Ghent University 1 Robbertverbekeugentbe Rbhfd Λ CDM Standard model for cosmology. 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. Rich Dwarf Galaxies. . Sambit. . Roychowdhury. (NCRA), . Jayaram. . N. . Chengalur. . (. NCRA. ), . . Igor . D. . Karachentsev. (SAO. ), Margarita . Sharina. (SAO). Ayesha Begum . Confronting Stellar Feedback . Simulations with Observations of Hot Gas in Elliptical Galaxies . Q. Daniel . Wang, . Shikui. Tang, Yu Lu, . Houjun. Mo . (UMass) . Mordecai . Mac-Low (AMNH. ), Ryan . Harry Ferguson (STScI). Feedback. Behroozi. + 2011. Halo quenching. Quasar mode AGN. Radio Mode AGN. (. SNe. ). SNe. Satellites: Ram pressure, tides, shocks…. UV back-ground. AGN feedback in . SAMs. Li Jiang-Tao. 1. Service d’Astrophysique, CEA, Saclay, France. 2. . Department. of . Astronomy. , . University. of Michigan, Ann Arbor, USA. Outline. 1. Introduction. 2. Diffuse X-ray . observation. 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. Megan Johnson. NRAO, Green Bank. Tully-Fisher Workshop, April 2012. Outline. Introduction. NGC 1569. Review of stellar and gas . kinematics from LITTLE THINGS. GBT map . NGC . 4163/NGC . 4214. Future Work. 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 . Confronting Stellar Feedback . Simulations with Observations of Hot Gas in Elliptical Galaxies . Q. Daniel . Wang, . Shikui. Tang, Yu Lu, . Houjun. Mo . (UMass) . Mordecai . Mac-Low (AMNH. ), Ryan . 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). diffuse X-ray emission – a survey of highly inclined disk galaxies. How is the emission correlated with galaxy properties?. How . are observations compared to simulations. ?. Nature of the emission – X-ray line spectroscopy. Oleg . Gnedin. (University of Michigan. ). g. raduate student . Hui. Li. Star clusters are dominant components of active star formation:. they connect small-scale SF (local) and global processes in galaxies. 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.

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