PPT-Astrophysical Evidence on

Heavy and Light Species Annika Peter Center for Cosmology and AstroParticle Physics CCAPP The Ohio State University HowWeScience on Instagram and Twitter Whoooo are youooh oohooh ooh. TSS-1 Smithsonian Astrophysical Observatory Tethers In Space HandbookM.L. Cosmo and E.C. LorenziniSmithsonian Astrophysical ObservatoryGrant NAG8-1160 monitored by C.C. RuppThe Smithsonian Astrophysic Acceleration Mechanisms. 1. Acceleration Mechanisms. There is clear observational evidence that hadrons and electrons are accelerated to extreme energies by astrophysical objects. direct evidence: charged cosmic rays. Primordial. or . Astrophysical. ?. Jungyeon. Cho. Chungnam. National . University, Korea. Cho & . Yoo. (2012; . ApJ. ). Cho (2013; PRD). Cho (2014, . ApJ. ). Origin of Magnetic fields in the ICM. CHARLES GREELEY ABBOTtories, including Harvard, Yerkes, and Lick. American as- CHARLES GREELEY ABBOT2/2 Abbot paid close attention to detail.to build a sturdy field station on the summit of MountWhitn Whipple was born November 5, 1906 in Red Oak, Iowa. He majored in mathematics at the University of California at Los Angeles. Then he went on to get his PhD in Astronomy at the University of California at Berkeley. Neutrino . L. imits. Georg G. Raffelt, Max-Planck-Institut f. ür Physik, München. Sun. Globular Cluster. Supernova 1987A. Cosmology. Questions about Neutrinos. Standard properties of active neutrinos. 2 show a chain of more or less regularly spaced emission knots which in some cases move at high speeds away from the central source; (iv) often terminate in emission lobes (with line emission in the c Astrophysical Fine Tuning, Naturalism, and the Contemporary Design Mark A. Walker and Milan M. Cacute] cacute]CISP_A_196002.sgmEvidence for instances of astrophysical Axion . L. imits. Georg G. Raffelt, Max-Planck-Institut f. ür Physik, München. Sun. Globular Cluster. Supernova 1987A. Dark Matter. Axion Bounds and Searches. Too . much CDM. (misalignment). Tele. Jonathan Carroll-Nellenback. Center for Integrated Research Computing. University of Rochester. Turbulence Workshop. August 4. th. 2015. Talk Outline. . Introduction to Turbulence in the context of gaseous flows. Siming. Liu. University of Glasgow. Collaborators. Vahe. ’ . Petrosian. , . Yanwei. Jiang: Stanford University. Zhonghui. Fan: Yunnan University. Oct. 2008 Krakow, Poland . Outline. I: Observations: Distribution. 1. John Beacom, The Ohio State University. High Energy . Neutrino . Astronomy. Topic: Impossible. Requires. : sources that reach high energies. . sources that are luminous. . sources of different types. axion. -photon . coupling. Oscar . Straniero. . . Italian National Institute of Astrophysics . . and INFN LNGS (Italy). Adrian Ayala. . Granada & Rome Universities (Spain/Italy). Maurizio . This compilation of data on deep-sky objects covers Messier objects, New General Catalogue objects and Index Catalogue objects. These are classified as galaxies, clusters and nebulae of which 500 individual objects are listed. Observing the deep-sky beyond the limits of the Solar System is by far the most popular speciality for amateur astronomers. Two major catalogs of deep-sky objects are widely used: Messier\'s catalogue of 109 objects and the New General Catalog (NGC) which contains thousands of objects. This catalog has entries for each of more than 500 deep-sky objects - all the Messier objects plus selected NGC objects. As well as the usual astronomical data they also detail physical factors, astrophysical information, evolution, ans unusual features. The objects are all listed in NGC order, which were originally assigned in approximate order of location from west to east, convenient for reference because objects that can be seen on a given night will occur within a few pages of each other in the book.