Category Archives: Uncategorized

Emission in Local Luminous Infrared Galaxies]​ Extended [CII] Emission in Local Luminous Infrared Galaxies Authors: T. Diaz-Santos, L. Armus, V. Charmandaris, G. Stacey, E. J. Murphy, S. Haan, S. Stierwalt, S. Malhotra, P. Appleton, H. Inami, G. E. Magdis, D. … Continue reading →

In the interest of motivating new thoughts in my head I’ve decided to prioritize actually reading something. I’ve been keeping a list of papers that I intended to read, largely from Hot Topics. I thought I would post them incase … Continue reading →

Three papers today. First, the environment dependence of SF in the center of IC342 looks at Xco and what causes it to vary. The abstract indicates that Xco varies with sigma H2, and that it agrees with theoretical predictions, so … Continue reading →

Very cool: http://www.sci-news.com/astronomy/science-star-forming-galaxy-primordial-hydrogen-01434.html

Cold dust but warm gas in the unusual elliptical galaxy NGC 4125 C. D. Wilson, A. Cridland, K. Foyle, T. J. Parkin, E. Mentuch Cooper, H. Roussel, M. Sauvage, M. W. L. Smith, M. Baes,G. Bendo, M. Boquien, A. Boselli, … Continue reading →

Low Masses and High Redshifts: The Evolution of the Mass-Metallicity Relation Alaina Henry, Claudia Scarlata, Alberto Dominguez, Matthew Malkan, Crystal L. Martin, Brian Siana, Hakim Atek, Alejandro G. Bedregal, James W. Colbert, Marc Rafelski, Nathaniel Ross,Harry Teplitz, Andrew J. Bunker, … Continue reading →

Hi all, here’s the X(CO) review by Bolatto, Wolfire and Leroy that we’re going to talk about for next week’s group meeting. -Alison 1301.3498v3.pdf

The first author can only be trusted so far. For one, Section 2.3 fails to mention a certain contributing grad student that helped with the NGC628 IRS data. For another, he’s short and his hair is too awesome. He’s dead … Continue reading →

Recently in our circle we have been repeatedly discussing that the centers of galaxies are typically dominated by older stellar populations, resulting in a very ‘red’ energy distribution. However, Dewitt et. al. uses near-infrared spectroscopy to identify three x-ray sources … Continue reading →

Two MIR color selected evolutionary studies, on hot dust, and radio AGN. JD Hot-Dust (690K) Luminosity Density and its Evolution in the last 7.5Gyr Hugo Messias, Bahram Mobasher, José Manuel Afonso (Submitted on 21 Aug 2013) [Abridged] We study the … Continue reading →