Amy Jones
University of Alabama
6 Papers
37 Citations
Amy Jones is an academic researcher from University of Alabama. The author has contributed to research in topics: Galaxy & Stellar mass. The author has an hindex of 4, co-authored 6 publications. Previous affiliations of Amy Jones include Texas A&M University.
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Papers
The Effect of Bars on the Ionized ISM: Optical Emission Lines from Milky Way Analogs
Dhanesh Krishnarao,Christy Tremonti,Amelia Fraser-McKelvie,Katarina Kraljic,Nicholas Fraser Boardman,Karen L. Masters,Robert A. Benjamin,L. Matthew Haffner,Amy Jones,Zachary J. Pace,Gail Zasowski,Matthew A. Bershady,Dmitry Bizyaev,Jonathan Brinkmann,Joel R. Brownstein,Niv Drory,Kaike Pan,Kai Zhang +17 more
TL;DR: Krishnarao et al. as mentioned in this paper used integral field spectroscopy to study the ionized gas conditions of 240 barred and 250 non-barred galaxies, focusing on those that are most similar to the Milky Way.
SDSS-IV MaNGA: Evidence for Enriched Accretion onto Satellite Galaxies in Dense Environments
Adam L. Schaefer,Christy Tremonti,Zachary J. Pace,Francesco Belfiore,Maria Argudo-Fernández,Matthew A. Bershady,Niv Drory,Amy Jones,Roberto Maiolino,David V. Stark,David Wake,Renbin Yan +11 more
TL;DR: In this paper, the authors investigate the environmental dependence of the local gas-phase metallicity in a sample of star-forming galaxies from the MaNGA survey and find that galaxies with stellar masses in the range $9 10^{10.5} \, \mathrm{M_{\odot}}$) centrals are more metal rich than satellites of low-mass centers, controlling for local stellar mass surface density and gas fraction.
Integrated Optical Polarization of Nearby Galaxies
TL;DR: In this paper, the authors performed an integrated optical polarization survey of 70 nearby galaxies to study the relationship between linear polarization and galaxy properties and found that dust scattering is the main source of optical polarization.
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Integrated Optical Polarization of nearby Galaxies
TL;DR: In this paper, the authors performed an integrated optical polarization survey of 70 nearby galaxies to study the relationship between linear polarization and galaxy properties and found that dust scattering is the main source of optical polarization.
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SDSS-IV MaNGA: Evidence for enriched accretion onto satellite galaxies in dense environments
Adam L. Schaefer,Christy Tremonti,Zachary J. Pace,Francesco Belfiore,Maria Argudo-Fernández,Matthew A. Bershady,Niv Drory,Amy Jones,Roberto Maiolino,David V. Stark,David Wake,Renbin Yan +11 more
TL;DR: In this paper, the authors investigate the environmental dependence of the local gas-phase metallicity in a sample of star-forming galaxies from the MaNGA survey and find that galaxies with stellar masses in the range $9 10^{10.5} \, \mathrm{M_{\odot}}$) centrals are more metal rich than satellites of low-mass centers, controlling for local stellar mass surface density and gas fraction.