(2015). Detection of HI in Emission in the Lyman Alpha Emitting ... Stephen A Pardy, John M Cannon, Göran Östlin, Matthew Hayes, et al. The Astronomical Journal endobj > This is the "surface" you'll see when you first go into his class, but beware of the dangers that lie below. Science has never been my strong suit and so I was worried about taking his astronomy class but the way he taught it made it so much easier. The main goal is to understand how \lya radiation is transported within galaxies: what fraction of it escapes, and what physical properties affect the \lya morphology and radiative transport (e.g., dust and gas content, metallicity, kinematics, properties of the producing and underlying stellar populations). Physics Commons, Home | endobj Max Planck Institute for Astronomy.

James has 8 jobs listed on their profile. Macalester College Segments of each research program are well-suited for undergraduate participation; please contact me if you are interested in learning more!

The Survey of Hi in Extremely Low-mass Dwarfs is an on-going multi-wavelength program to characterize the gas, star formation, and ... (Almost) Dark HI Sources in the ALFALFA Survey: The Intriguing ... Steven Janowiecki, Lukas Leisman, Gyula Jozsa, John J. Salzer, et al. John Cannon. endobj John CANNON of Macalester College, Saint Paul | Read 162 publications | Contact John CANNON

He is clear, emphasizes concepts well, and is unafraid to spend a lot of time easing confusion. School Counselors, Kristine I. Spangard, Department Coordinator. <>

651-696-6000, Parents &

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application/pdf View Photos. Paul, MN 55105651) 696-6122. John is the best professor I've had at Mac so far. HI Observations of the Local Group Dwarf WLM John Cannon is passionate about his material. AppendPDF Pro 5.5 Linux Kernel 2.6 64bit Oct 2 2014 Library 10.1.0 Killer professor, great class. Aid & Tuition, Admitted The hard part is his long tests, which are tough if you are a slower worker. 2017-08-25T07:35:49Z Insists on being called "John", which is a really nice informality.

<>stream 69117 Heidelberg E. A.K. LARS09 has a severely disturbed optical morphology; our new \HI observations reveal that LARS09 is interacting with the nearby field galaxy SDSS J082353.65+280622.2. His thesis work was in extragalactic observational astronomy, with an emphasis on the panchromatic properties of starbursts in Dwarf Galaxies. Admissions, International

2017-08-25T07:35:49Z Erik D. Alfvin, Brendan P. Miller, M. P. Haynes, E. Gallo, et al. Abstract. 1 (2017), A Direct Comparison of Lyman-Alpha and Neutral Hydrogen Morphologies, Kathleen Fitzgibbon, Macalester CollegeFollow endobj Images of the \HI mass surface density and of the intensity weighted \HI velocity field were created at angular scales of $\sim$8 arcseconds, which corresponds to $\sim$5 kpc for LARS02 and $\sim$8 kpc for LARS09. This is NOT an intro class. Morphology at Low and ... L. Guaita, J. Melinder, M. Hayes, G. Ostlin, et al. It is offered for first year students, but the level of work seems to be closer to a junior/senior level course. The Lyman Alpha Reference Sample: V. Empirical Inferences on the ... T. E. Rivera-Thorsen, M. Hayes, G. Ostlin, F. Duval, et al. Admissions, For High 5 endobj Characterizing the Star Formation of the Low-Mass SHIELD Galaxies from ... K. B.W. The resulting datasets have yielded a comprehensive suite of multiwavelength diagnostics of these intriguing galaxies. They provide an opportunity to study star formation processes, stellar populations and chemical evolution in unprecedented detail. gF/(+GaKo$qneLWDrQ#;5\S(\$q'4Q,85`-8;S(=Z"WSBOV*FM)4,?B],R I wouldn't recommend taking a class from him unless you're really interested in astronomy. These observations demonstrate concept for a significant observational campaign to produce similar comparisons in the remaining 40 LARS and eLARS galaxies. He gives difficult tests, but grades as fairly as possible. 1 0 obj Families, U.S. 66 0 obj John Cannon, 43 Minneapolis, MN. The frequency and properties of young tidal dwarf galaxies in ... K. Lee-Waddell, K. Spekkens, P Chandra, N Patra, et al. John M Cannon, C. P. Martinkus, L. Leisman, M. P. Haynes, et al. <>

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