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Maxwell Moe

Researcher at University of Colorado Boulder

Publications -  7
Citations -  671

Maxwell Moe is an academic researcher from University of Colorado Boulder. The author has contributed to research in topics: Quasar & Outflow. The author has an hindex of 5, co-authored 7 publications receiving 642 citations.

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Quasar Outflow Contribution to AGN Feedback: Observations of QSO SDSS J0838+2955

TL;DR: In this paper, a detailed analysis of the Astrophysical Research Consortium 3.5 m telescope spectrum of QSO SDSS J0838+2955 was presented, showing three broad absorption line (BAL) systems at 22,000, 13,000 and 4900 km s{sup -1} blueshifted from the systemic redshift of z = 2.043.
Journal ArticleDOI

Quasar Outflow Contribution to AGN Feedback: Observations of QSO SDSS J0838+2955

TL;DR: In this paper, a detailed analysis of the Astrophysical Research Consortium 3.5 m telescope spectrum of QSO SDSS J0838+2955 was presented, showing three broad absorption line (BAL) systems at 22,000, 13,000 and 4900 km s^-1 blueshifted from the systemic redshift of z=2.043.
Journal ArticleDOI

Measuring Column Densities in Quasar Outflows: VLT Observations of QSO 2359–1241*

TL;DR: In this paper, high-resolution spectroscopic VLT observations of the outflow seen in QSO 2359-1241 were used to investigate the physical distribution of the material in front of the source and by that to determine the column densities of the absorbed troughs.
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Physical Conditions in Quasar Outflows: Very Large Telescope Observations of QSO 2359-1241*

TL;DR: In this paper, the physical conditions of the outflow seen in QSO 2359-1241 (NVSS J235953-124148) were analyzed based on high-resolution spectroscopic VLT observations.
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Distance to Multiple Kinematic Components of Quasar Outflows: Very Large Telescope Observations of QSO 2359-1241 and SDSS J0318-0600

TL;DR: In this paper, the authors studied the multi-component outflow systems of two quasars exhibiting intrinsic Fe II absorption (QSO 2359-1241 and SDSS J0318-0600) using high-resolution Very Large Telescope spectra.