PPT-Investigating the Low-Mass Stellar Initial Mass Function in

Author : myesha-ticknor | Published Date : 2016-07-19

Soroush Sotoudeh University of Minnesota Daniel Weisz Andrew Dolphin Evan Skillman 06292015 STScI Workshop on IMF Outline Introduction Observations and data

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Investigating the Low-Mass Stellar Initial Mass Function in: Transcript


Soroush Sotoudeh University of Minnesota Daniel Weisz Andrew Dolphin Evan Skillman 06292015 STScI Workshop on IMF Outline Introduction Observations and data IMF analysis and results. Driven Outflows in Cosmological Galaxy Evolution. Ben Keller (McMaster University). James . Wadsley. , Hugh . Couchman. CASCA 2015. Paper. : . astro-ph. : 1505.06268. Keller, . Wadsley. & . Couchman. Galaxies. T.Naab. , P. Johansson, R. . Cen. , K. . Nagamine. , R. . Joung. . and J.P.O.. PPPL:, 19 Dec . 2012. ApJ.L.,. 658,710 . (2007) ApJ.,697, . 38 . (2009). ApJ.L.,699,L178 (. 2009. ). ApJ.,725,2312 . 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. . Metallicity. Relation at High . Redshifts. Stellar-mass . Metallicity. Relation at . z~. 1.. 4. Kouji. OHTA.  (. Kyoto University. ). K. Yabe. , F. . Iwamuro. , S. Yuma, M. Akiyama, N. Tamura, FMOS team et al.. . Technique. . for. . the. . Determination. . of. IMF . at. . Low. . Masses. : . A. . Few. . Results. . for. . Galaxies. . with. Old. . Stellar. . Populations. Nikolay. Podorvanyuk. 1. Scott Croom. Julia Bryant. Joss Bland-Hawthorn. Disturbed Things Come in . small. packages. Jessica V. Bloom. Kinematics can uncover processes shaping galaxy evolution. Bloom et al., 2016 (submitted). 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 . Steven R. . Cranmer. Harvard-Smithsonian Center for . Astrophysics. . with A. van . Ballegooijen. , S. Saar, A. Dupree, N. . Brickhouse. , et al.. Stellar winds across the H-R Diagram. Massive stars: radiation-driven winds. Multi-. Scale . Environmental . Influences on Galaxy Gas Content. Environmental processes can influence galaxy gas content. “Small” (dark matter halo) scale. Gas replenishment. c. osmological accretion. Daisuke Suzuki. ISAS / JAXA. the MOA collaboration. August . 8. , 2017 . 2017 Sagan Summer Workshop. Microlensing in the Era of WFIRST . a. snow. . = 2.7 (. M. /. M. Sun. ) AU. http://. exoplanet.eu. Ben Keller (McMaster University). James . Wadsley. , Hugh . Couchman. CASCA 2015. Paper. : . astro-ph. : 1505.06268. Keller, . Wadsley. & . Couchman. 2015. Background Image: Gas column density of IGM around a simulated . N. . Prantzos. Lecturer:. . Hans-Jürgen . Wollersheim. e-mail: . h.j.wollersheim@gsi.de. web-page: . https://web-docs.gsi.de/~. wolle/. and click on . thermodynamics. subatomic physics. Sun´s energy. Learning Intentions . Properties of Stars. In this topic we are going to examine: . temperature and colour of a star. spectral class. the power of a star. stellar luminosity. apparent brightness. symbols. CIERA postdoctoral fellow. the stellar progenitors of long-duration gamma ray bursts. MICRA 2023. ECT*, Trento, IT. september 10, 2023. iron core. (stripped) stellar envelope. gravitational collapse.

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