On the Radiative Acceleration of Quasar Absorption Line Clouds
Radiation may expel dense gas clouds from quasar emission line regions. Small clouds can be accelerated to velocities approaching c if they are confined so as to maintain high densities.
Goldreich, Peter
core
The emission-line regions in broad absorption line quasars
G. F. Hartig, J. A. Baldwin
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Unexpected silicon localization in calcium carbonate exoskeleton of cultured and fossil coccolithophores. [PDF]
Bordiga M +18 more
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First rest-frame infrared spectrum of a z > 7 quasar: MIRI-MRS observations of J1120+0641
Bosman S +31 more
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The radio properties of the broad absorption-line quasars
J. T. Stocke +3 more
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Robust and Democratic s‑SNOM Data Analysis and Modeling in Quasar. [PDF]
Németh G +4 more
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Morphological and lipid metabolism alterations in macrophages exposed to model environmental nanoplastics traced by high-resolution synchrotron techniques. [PDF]
Zingaro F +9 more
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AXZ viewer: a web application to visualize unprocessed AFM-IR data. [PDF]
Duverger W +4 more
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Radio Properties of Broad Absorption Line Quasars
学位の種別:課程博士 審査委員会委員 : (主査)東京大学教授 坪井 昌人, 東京大学准教授 梅田 秀之, 東京大学教授 海老沢 研, 東京大学教授 家 正則, 山口大学教授 藤沢 ...
openaire
Possible nonstellar explanation for the unexpected brightness of the earliest galaxies observed by the James Webb Space Telescope. [PDF]
Jacak JE.
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