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spectrum - Columbia Astrophysics Laboratory

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RAY J. WEYMANN. Steward Observatory, University of Arizona. FREDERIC H. CHAFFEE, JR. Mount Hopkins Observatory; and Smithsonian Astrophysical Observatory. › twin_spectra

Ray Weymann - The Mathematics Genealogy ProjectThe Mathematics Genealogy Project

genealogy.math.ndsu.nodak.edu

Ray J. Weymann. Dissertation: Advisor: Unknown. Student: Name, School, Year, Descendants. Peterson, Bradley, University of Arizona,

Absorption lines in the spectra of quasistellar objectsNASA/ADS

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von RJ Weymann · · Zitiert von: 386 — ... J. Weymann Steward Observatory, University of Arizona, Tucson, Arizona Robert F. Carswell Institute of Astronomy, Cambridge University, Cambridge ... von RJ Weymann · · Zitiert von: 386 — ... J. Weymann Steward Observatory, University of Arizona, Tucson, Arizona Robert F. Carswell Institute of Astronomy, Cambridge University, Cambridge ...

THE ORIGIN OF ABSORPTION SPECTRA IN QUASI- ...Internet Archive Scholar

scholar.archive.org

von RJ Weymann · · Zitiert von: 6 — Ray J. Weymann. Steward Observatory, University of Arizona. ABSTRACT. A classification scheme for QSO absorption line spectra is described which ascribes the ... von RJ Weymann · · Zitiert von: 6 — Ray J. Weymann. Steward Observatory, University of Arizona. ABSTRACT. A classification scheme for QSO absorption line spectra is described which ascribes the ...

THEORETICAL ASPECTS OF MASS LOSS FROM LATE- ...Internet Archive Scholar

scholar.archive.org

von RJ Weymann · Zitiert von: 3 — THEORETICAL ASPECTS OF MASS LOSS FROM LATE-TYPE STARS. Ray J. Weymann. Steward Observatory. University of Arizona. Tucson, Arizona U.S.A.. I. INTRODUCTION. von RJ Weymann · Zitiert von: 3 — THEORETICAL ASPECTS OF MASS LOSS FROM LATE-TYPE STARS. Ray J. Weymann. Steward Observatory. University of Arizona. Tucson, Arizona U.S.A.. I. INTRODUCTION.

Electron-Scattering Line Profiles in Nuclei of Seyfert Galaxies

adsabs.harvard.edu

von RJ Weymann · · Zitiert von: 54 — Printed in U.S.A. ELECTRON-SCATTERING LINE PROFILES IN NUCLEI OF SEYFERT GALAXIES R~x J. WEYMANN Steward Observatory, University of Arizona Received › full

The Discovery of a Gravitational LensJstor

www.jstor.org

von FH Chaffee · · Zitiert von: 18 — Carswell of the University of. Cambridge and Ray J. Weymann of the University of Arizona discovered two quasars separated by only six sec onds of arc, an ... von FH Chaffee · · Zitiert von: 18 — Carswell of the University of. Cambridge and Ray J. Weymann of the University of Arizona discovered two quasars separated by only six sec onds of arc, an ...

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J. Weymann und University Of Arizona Person-Info

spectrum - Columbia Astrophysics Laboratory

Ray Weymann - The Mathematics Genealogy ProjectThe Mathematics Genealogy Project

Absorption lines in the spectra of quasistellar objectsNASA/ADS

THE ORIGIN OF ABSORPTION SPECTRA IN QUASI- ...Internet Archive Scholar

THEORETICAL ASPECTS OF MASS LOSS FROM LATE- ...Internet Archive Scholar

Electron-Scattering Line Profiles in Nuclei of Seyfert Galaxies

The Discovery of a Gravitational LensJstor

THE AUTHORSJSTOR

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Quasar Image Split by Gravity Is ReportedThe New York Times

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