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IRAC/MIPS view of the ISM: PAHs dominate in IRAC Li & Draine (2001) dust emissivity model; only very strong (> 10 3 x avg.) radiation fields contribute.
Documents IRAC/MIPS view of the ISM: PAHs dominate in IRAC Li & Draine (2001) dust emissivity model; only very...

Slide 1 IRAC/MIPS view of the ISM: PAHs dominate in IRAC Li & Draine (2001) dust emissivity model; only very strong (> 10 3 x avg.) radiation fields contribute to…

Susan CartwrightOur Evolving Universe1 Other galaxies n Telescopic images of the night sky reveal many other galaxies l l What do they look like? are.
Documents Susan CartwrightOur Evolving Universe1 Other galaxies n Telescopic images of the night sky reveal...

Slide 1 Susan CartwrightOur Evolving Universe1 Other galaxies n Telescopic images of the night sky reveal many other galaxies l l What do they look like?   are they…

M. Arnaboldi ICPNe as probes of diffuse light in clusters July 2 nd, 2005 Magda Arnaboldi, PNe as Astronomical Tools July 2 nd, 2005 Intracluster Planetary.
Documents M. Arnaboldi ICPNe as probes of diffuse light in clusters July 2 nd, 2005 Magda Arnaboldi, PNe as.....

Observations of Diffuse Light Intracluster Light in Cosmological Simulations ICPNe in the Virgo Cluster: projected phase-space distribution Future prospects 1951. Zwicky…

Galaxy Luminosity Function (LF) – Φ (yes, another use of “phee”!) - What are the relative numbers of galaxies of different luminosities? δN = Φ(L) δL δV.
Documents Galaxy Luminosity Function (LF) – Φ (yes, another use of “phee”!) - What are the relative...

Slide 1 Galaxy Luminosity Function (LF) – Φ (yes, another use of “phee”!) - What are the relative numbers of galaxies of different luminosities? δN = Φ(L) δL δV…

Diffuse Light in Galaxy Groups Nieves D. Castro-Rodríguez 1, J. Alfonso L. Aguerri 1, Magda Arnaboldi 2, Ortwin Gerhard 3 1 Instituto de Astrofísica de.
Documents Diffuse Light in Galaxy Groups Nieves D. Castro-Rodríguez 1, J. Alfonso L. Aguerri 1, Magda...

Diffuse Light in Galaxy Groups Nieves D. Castro-Rodríguez1, J. Alfonso L. Aguerri1, Magda Arnaboldi2, Ortwin Gerhard3 1Instituto de Astrofísica de Canarias 2Osservatorio…

ETY 2006 ety@ece.ucsd.edu tel: +1.858.534.6619 fax: +1.858.822.3425 Nanoscale physics of nitride semiconductor heterostructures.
Documents ETY 2006 [email protected] tel: +1.858.534.6619 fax: +1.858.822.3425 Nanoscale physics of nitride...

Nanoscale physics of nitride semiconductor heterostructures for electronic and optoelectronic devices Our principal research objective is to elucidate the relationships among…

Radio Loudness of AGNs: Host Galaxy Morphology and the Spin Paradigm Łukasz Stawarz (KIPAC, Stanford University) Marek Sikora (CAMK, Poland) Jean-Pierre.
Documents Radio Loudness of AGNs: Host Galaxy Morphology and the Spin Paradigm Łukasz Stawarz (KIPAC,...

Radio Loudness of AGNs: Host Galaxy Morphology and the Spin Paradigm Łukasz Stawarz (KIPAC, Stanford University) Marek Sikora (CAMK, Poland) Jean-Pierre Lasota (IAP, France)…

Lecture 34 – Galaxies and the Universe
Documents Lecture 34 – Galaxies and the Universe

Lecture 34 â Galaxies and the Universe Repeatedly said there are other galaxies. Now details Large Magellanic Cloud (satellite to Milky Way) . Distance=50 kpc. Pic:http://antwrp.gsfc.nasa.gov/apod/ap010804.html…

Intracluster Planetary Nebulae as Dynamical Probes of the Diffuse Light in Galaxy Clusters
Documents Intracluster Planetary Nebulae as Dynamical Probes of the Diffuse Light in Galaxy Clusters

Observations of Diffuse Light Intracluster Light in Cosmological Simulations ICPNe in the Virgo Cluster: projected phase-space distribution Future prospects 1951. Zwicky…

Diffuse Light in Galaxy Groups
Documents Diffuse Light in Galaxy Groups

Diffuse Light in Galaxy Groups Nieves D. Castro-Rodríguez1, J. Alfonso L. Aguerri1, Magda Arnaboldi2, Ortwin Gerhard3 1Instituto de Astrofísica de Canarias 2Osservatorio…

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