'Flux densities' presentation slideshows

Solar System Objects

414 views • 36 slides

Solar System Objects

557 views • 35 slides

[ C II ] 158 m m Emission from Damped Ly a Systems

[ C II ] 158 m m Emission from Damped Ly a Systems. Art Wolfe and Ken Nagamine UCSD. DLAS are. Definition of Damped Ly a System (DLA): N(HI) > 2*10 20 cm -2 Distinguishing characteristic of DLAs : Gas is Neutral. DLAS are. Definition: N(HI) > 2*10 20 cm -2

294 views • 20 slides

THE PROBLEM

Space reconstruction of the morphology and kinematics of axisymmetric radio sources P.N. Diep*, N.T. Phuong, D.T. Hoai, P.T. Nhung, N.T. Thao, P.Tuan-Anh and P. Darriulat Department of Astrophysics (DAP) Vietnam National Satellite Center (VNSC) Quy Nhon, August 2016. THE PROBLEM

194 views • 19 slides

THE PROBLEM

Space reconstruction of the morphology and kinematics of axisymmetric radio sources P.N. Diep*, N.T. Phuong, D.T. Hoai, P.T. Nhung, N.T. Thao, P.Tuan-Anh and P. Darriulat Department of Astrophysics (DAP) Vietnam National Satellite Center (VNSC) Quy Nhon, August 2016. THE PROBLEM

193 views • 19 slides

OCRA-p science projects

OCRA-p science projects. Marcin Gawro?ski. Bonn 14.III.2011. Observations with OCRA-p - two modes of observations (for bright and weak sources ) - one primary flux density calibrator (NGC 7027, Hafez et al., 2008)

356 views • 17 slides

Investigating the radio emission from stellar and sub-stellar systems: How common is Coherent Emission?

Investigating the radio emission from stellar and sub-stellar systems: How common is Coherent Emission?. The TEAM: G. Umana 1 , O., B. Slee 2 , E. Budding 3 , A. Antonova 4 , D. Blank 5 , C. S. Buemi 1 , J. D. Bunton 11 , J.G. Doyle 6 ,

204 views • 6 slides