PPT-Extinction, emission and polarisation of dust

Large Interstellar Polarisation Survey Stefano Bagnulo Nikolai Voshchinnikov Nick Cox PI Dust extinction emission amp polarisation in the diffuse ISM Simultaneously model . of dust heating in M81, M83 and NGC 2403 with Herschel and Spitzer. George J. . Bendo. Very Nearby Galaxies Survey . Goals. The overall goals of this research are to empirically identify the heating sources for the dust observed at 70-500 µm.. JWST Workshop. – . STScI. Baltimore. June 8, 2011. Mid-Infrared Observation of High . Redshift. Galaxy Evolution. Most star formation activity occurs behind dust . Chary & Pope . 2011. Bouwens. Adam Leroy. National Radio Astronomy Observatory. HERITAGE (. Meixner. et al.). Dust in Dwarf Galaxies. Adam Leroy. National Radio Astronomy Observatory. HERITAGE (. Meixner. et al.). SAGE (. Meixner. Lecture 8: Dusty starburst galaxies. Prof.. . Dr.. M. . Baes. (. UGent. ). Prof.. . Dr.. C. . Waelkens. (KUL). Academic year 2015-2016. The interstellar medium. The space between the stars in a galaxy is not empty. WDs. . Jana Bilikova. 1. . . You-. Hua. Chu. 1. , Kate Su. 2. , Robert Gruendl. 1, . et al.. 1. U. of Illinois at Urbana-Champaign, . 2. U. of Arizona . . Spitzer MIPS 24 . μm. Survey of Hot . Increasing . the accessibility and mobility of toxic . metals. Dr.. James King. Acknowledgements. Richard Reynolds, Harland Goldstein, . Jim . Yount. , George . Breit. , Suzette . Morman. George Nikolich, Jack Gillies, Vic Etyemezian. in GRB Host Galaxies. Patricia Schady. (MPE). T.Dwelly. , . M.J.Page. , . J.Greiner. ,. T.Krühler. , . S.Savaglio. , . S.R.Oates. , . A.Rau. , . M.Still. + GROND and UVOT team. z. Number of . GRBs. RESEARCH. q. uality and quantity. Paul Dowling. Institute of Education. University of London. Photometric . redshifts. can be routinely obtained to accuracies of better than 0.1 in Deltaz/(1 +. z. ). The issue of dust extinction, however, is one that has still not been well quantified. In this paper the success of two template-fitting photometric . Bryan Gaensler. , Tom Landecker, Russ Taylor. and the POSSUM team. askap.org. /possum. New Discovery Space with ASKAP-12. Radio polarimetry: a highly sensitive probe of density, magnetic field and turbulence at all redshifts. Daniel Cotton (UNSW). with. Jeremy Bailey, Lucyna Kedziora-Chudczer, Kimberly Bott & Jonty Marshall. II. III. IV. V. Overview. Polarisation Basics. Stellar Polarimetry History. Why do people care about polarisation now: Exoplanets! . Electric susceptibility. Displacement field in matter. Boundary conditions on fields at interfaces. What . is the . macroscopic (average) electric field. inside matter when an external . E. field is applied. polarised. emission in X-ray binaries. Dave Russell. New York University Abu Dhabi. dave.russell@nyu.edu. In collaboration with T. ariq . Shahbaz. (IAC, Tenerife). I’d also like to thank Rob Fender, Elena Gallo, . Remember. Operant conditioning extinction differs from classical conditioning extinction. During extinction, responding decreases to baseline levels for both classical and operant conditioning. BUT: Operantly conditioned behavior shows:. ). (Section 18.2, bits of 18.7,18.8). Space between stars is not a . vacuum but. is filled with gas.. Why . is the ISM important? . Stars form out of it. Stars end their lives by returning gas to .