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Browsing by Author Jameson, Katherine

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01_Warren_Carma_CO_observations_of_three_2015.pdf.jpg

Carma CO observations of three extremely metal-poor, star-forming galaxies

Author(s)Warren, Steven R.; Molter, Edward M.; Cannon, John M., et al
TypeJournal article
Date Published2015
Date Created-
01_Rahman_Carma_survey_toward_2011.pdf.jpg

Carma survey toward infrared-bright nearby galaxies (STING): Molecular gas star formation law in NGC 4254

Author(s)Rahman, N.; Bolatto, Alberto; Wong, T, et al
TypeJournal article
Date Published2011
Date Created-
01_Gordon_Dust_and_gas_in_the_magellanic_2014.pdf.jpg

Dust and gas in the magellanic clouds from the heritage Herschel Key Project. I. Dust properties and insights into the origin of the submillimeter excess emission

Author(s)Gordon, Karl D.; Roman-Duval, Julia; Caroline, B. O. T., et al
TypeJournal article
Date Published2014
Date Created-
01_Roman-Duval_Dust_and_gas_in_the_magellanic_2014.pdf.jpg

Dust and gas in the magellanic clouds from the heritage herschel key project. II. Gas-to-dust ratio variations across interstellar medium phases

Author(s)Roman-Duval, Julia; Gordon, Karl D.; Meixner, Margaret, et al
TypeJournal article
Date Published2014
Date Created-
01_Hull_Misalignment_of_magnetic_2013.pdf.jpg

Misalignment of magnetic fields and outflows in protostellar cores

Author(s)Hull, Charles L.H.; Plambeck, Richard L.; Bolatto, Alberto, et al
TypeJournal article
Date Published2013
Date Created-
01_Jameson_THE_RELATIONSHIP_BETWEEN_2016.pdf.jpg

THE RELATIONSHIP BETWEEN MOLECULAR GAS, H I, AND STAR FORMATION IN THE LOW-MASS, LOW-METALLICITY MAGELLANIC CLOUDS

Author(s)Jameson, Katherine; Bolatto, Alberto; Leroy, Adam K., et al
TypeJournal article
Date Published2016
Date Created-
01_Bolatto_The_state_of_the_gas_and_the_2011.pdf.jpg

The state of the gas and the relation between gas and star formation at low metallicity: The small magellanic cloud

Author(s)Bolatto, Alberto; Leroy, Adam K.; Jameson, Katherine, et al
TypeJournal article
Date Published2011
Date Created-
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