M
Max Moe
Researcher at Harvard University
Publications - 4
Citations - 270
Max Moe is an academic researcher from Harvard University. The author has contributed to research in topics: Extinction (astronomy) & Luminosity. The author has an hindex of 3, co-authored 4 publications receiving 255 citations. Previous affiliations of Max Moe include University of Colorado Boulder.
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Journal ArticleDOI
The quasar outflow contribution to agn feedback: vlt measurements of sdss j0318-0600*
Jay P. Dunn,Manuel A. Bautista,Manuel A. Bautista,Nahum Arav,Max Moe,Max Moe,Kirk T. Korista,Elisa Costantini,Chris Benn,Sara L. Ellison,Doug Edmonds +10 more
TL;DR: In this article, high-resolution Very Large Telescope observations of the broad absorption line quasar SDSS J0318-0600 were used to extract accurate ionic column densities and determine an electron number density of ne = 103.3±0.2 cm−3 for the main outflow absorption component.
Journal ArticleDOI
The Quasar Outflow Contribution to AGN Feedback: VLT Measurements of SDSS J0318-0600
Jay P. Dunn,Manuel A. Bautista,Manuel A. Bautista,Nahum Arav,Max Moe,Max Moe,Kirk T. Korista,Elisa Costantini,Chris Benn,Sara L. Ellison,Doug Edmonds +10 more
TL;DR: In this article, high spectral resolution VLT observations of the BAL quasar SDSS J0318-0600 were used to extract accurate ionic column densities and determine an electron number density of n_e=10^3.
Journal ArticleDOI
DETERMINING THE LOCATIONS OF DUST SOURCES IN FeLoBAL QUASARS
Jay P. Dunn,Branden Wasik,Christin L. Holtzclaw,David Yenerall,Manuel A. Bautista,Nahum Arav,Daniel Hayes,Max Moe,Luis C. Ho,Luis C. Ho,S. Harper Dutton +10 more
TL;DR: In this article, the authors conduct a spectroscopic search of quasars observed by the Sloan Digital Sky Survey (SDSS) with broad absorption line (BAL) troughs due to Mg ii and Fe ii that simultaneously exhibit strong Balmer narrow emission lines (NELs).
Journal ArticleDOI
Determining the Locations of Dust Sources in FeLoBAL Quasars
Jay P. Dunn,Branden Wasik,Christin L. Holtzclaw,David Yenerall,Manuel A. Bautista,Nahum Arav,Daniel Hayes,Max Moe,Luis C. Ho,Luis C. Ho,S. Harper Dutton +10 more
TL;DR: In this article, the authors conduct a spectroscopic search of quasars observed by the Sloan Digital Sky Survey (SDSS) and find that in a redshift range of 0.4 less than or equal to z less than and equal to 0.9 approximately 23 of the 70 Mg II BALs and 4 of a subset of 15 Fe II emission lines exhibit strong Balmer emission.