'Thermal emission' presentation slideshows

Lecture 7

Lecture 7. Continuum Emission in AGN. UV-Optical Continuum. Infrared Continuum. High Energy Continuum. Radio Continuum - Jets and superluminal motion.

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The Zoo Of Neutron Stars

The Zoo Of Neutron Stars. Sergei Popov ( SAI MSU ). ( www.bradcovington.com). JINR, Dubna, August 30, 2006. Main reviews. NS basics : physics/0503245 SGRs & AXPs: astro-ph/040613 Magnetars : - Observations astro-ph/0505491 - Theory astro-ph/0504077 Central compact X-ray

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Supernova Remnants and their Emission

Supernova Remnants and their Emission. Aya Bamba (Aoyama Gakuin U.). ??????? ????. Member of astro group in Aoyama Gakuin Univ. ?? ?? ?????????????????????? ??????????????????????????????? ?? ? ???????? ???????????????????? ????????? ??????????????? SNR ? CTA ? CALET

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Astronomical Observational Techniques and Instrumentation

Astronomical Observational Techniques and Instrumentation. RIT Course Number 1060-771 Professor Don Figer Radio Astronomy. Aims of Lecture. review radio imaging chain describe radio sources describe radio detection describe some common radio telescopes give examples of radio objects.

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Interstellar medium

Roberto Decarli. Interstellar medium. - What is the ISM? - Emission and absorption - Electromagnetic wave propagation - Structure and other astronomical hints - Computational models. Extragalactic Astronomy A.Y. 2004-2005. What is the ISM?.

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CHARM Telecon June 30, 2009 Saturn Interior and Atmosphere

CHARM Telecon June 30, 2009 Saturn Interior and Atmosphere. Andrew Ingersoll, Caltech Saturn Discipline Working Group This talk was originally presented at the Cassini Solstice Mission Senior Review on February 10, 2009. XXM Prioritized Objectives for Saturn.

360 views • 29 slides

Fermi Bubble

Fermi Bubble. Z.G.,Xiong. Outline. Observations Theories Simulations Discussion. Observations. Finkbeiner,2004. Bland-Hawthorn & Cohen, 2003. Su et al .,2010. Characteristics: size symmetry uniform common origin morphology spectrum. Theories. Bipolar Galactic wind

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Galactic diffuse

Galactic diffuse. ? Thermal emission from SNRs/SNe ? Miyata 35min ? Non-thermal emission from SNRs/SNe ? Ozaki 15min ????????? X ???? Torii 15min ????????????? X ???????? Torii 10min ???????????????? AXP ? SGR ??? Torii 15min ????? / ??????? diffuse ?? Kokubun 15min

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Oceanic Whitecaps: Good or Bad?

Bridging the Gap October 21 - 22 , 2000. Oceanic Whitecaps: Good or Bad?. Magdalena Anguelova. Good or Bad for Remote Sensing. The role of whitecaps The characteristics of whitecaps Judging the whitecaps. Good or Bad for Remote Sensing. The role of whitecaps. Climate Changes.

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Spitzer Observations of 3C Quasars and Radio Galaxies:

Spitzer Observations of 3C Quasars and Radio Galaxies: Mid-Infrared Properties of Powerful Radio Sources. K. Cleary 1 , C.R. Lawrence 1 , J.A. Marshall 2 , L. Hao 2 , D. Meier 1. 1: JPL, California Institute of Technology 2: Cornell University. Summary. Why observe in infrared? Previous Work

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Direct Photon Production at RHIC

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Feb. 2, 2011 Rosseland Mean Absorption Poynting Vector Plane EM Waves The Radiation Spectrum: Fourier Transforms

Feb. 2, 2011 Rosseland Mean Absorption Poynting Vector Plane EM Waves The Radiation Spectrum: Fourier Transforms. Rosseland Mean Opacity. Recall that for large optical depth . In a star, . is large, but there is a temperature gradient. Plane parallel atmosphere.

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Rosseland Mean Opacity

Feb. 2, 2011 Rosseland Mean Absorption Poynting Vector Plane EM Waves The Radiation Spectrum: Fourier Transforms. Rosseland Mean Opacity. Recall that for large optical depth. In a star,. is large, but there is a temperature gradient. Plane parallel atmosphere.

336 views • 22 slides

Synergy of Gamma-ray and (mm-) Radio O bservations in Studying M olecular Clouds

Synergy of Gamma-ray and (mm-) Radio O bservations in Studying M olecular Clouds. July 23, 2014@Nobeyama T. Mizuno (Hiroshima Astrophysical Science Center). ??? ?? ??????????? ( ??? ) ???????. July 23, 2014@Nobeyama T. Mizuno (Hiroshima Astrophysical Science Center).

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Towards an Understanding of the Isolated Neutron Star RX J1856.5-3754

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Geometry of acceleration in the bipolar remnant of SN1006 with XMM-Newton

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EUV and HXR evidence of chromospheric evaporation in a solar flare

EUV and HXR evidence of chromospheric evaporation in a solar flare. NING Zongjun Purple Mountain Observatory. 2007 Dec. 14 C1.1 flare joint observed by RHESSI, Hinode/EIS and TRACE. RHESSI 12-25 keV.

232 views • 11 slides

B-Pol Satellite experiment: HWP technologies comparison

B-Pol Satellite experiment: HWP technologies comparison. The University of Manchester. Giampaolo Pisano Radioastronomy Technology Group Jodrell Bank Centre for Astrophysics, University of Manchester, UK B-Pol Meeting - Paris, 29-30 July 2010. Half-Wave Plates: Requirements.

211 views • 10 slides

Ground-Based Detections of Thermal Emission from Very Hot Jupiters

Direct detection of flux from planet from secondary eclilpse depth Hottest planets: thermal emission dominates - depends on albedo, energy redistribution Spitzer obs. reveal fundamental dichotomy pM: optical absorbers, thermal inversion (hot stratosphere)

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Objectives Evaluate effects of underlap (L d ) Evaluate effects of boundary condition Methods

Effects of Underlap and Boundary Condition Zhengping Jiang, Yeqing Lu, Yaohua Tan, Yu He, Michael Povoloskyi , Tillmann Kubis, Alan Seabaugh , Patrick Fay, Gerhard Klimeck. Objectives Evaluate effects of underlap (L d ) Evaluate effects of boundary condition Methods

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