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Wednesday, May 6, 2020 | History

2 edition of Structure of the K-Line During the Ingress Phase of the 1961 Eclipse of 31 Cygni. found in the catalog.

Structure of the K-Line During the Ingress Phase of the 1961 Eclipse of 31 Cygni.

Canada. Dept. of Mines and Technical Surveys. Dominion Observatories.

Structure of the K-Line During the Ingress Phase of the 1961 Eclipse of 31 Cygni.

by Canada. Dept. of Mines and Technical Surveys. Dominion Observatories.

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  • 36 Currently reading

Published by s.n in S.l .
Written in English


Edition Notes

1

SeriesCanada Dominion Astrophysical Observatory Contributions -- 77
ContributionsWright, K.O.
ID Numbers
Open LibraryOL21904325M


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Structure of the K-Line During the Ingress Phase of the 1961 Eclipse of 31 Cygni by Canada. Dept. of Mines and Technical Surveys. Dominion Observatories. Download PDF EPUB FB2

The ζ Aurigae system 31 Cygni (K4 Ib + B4 V) was observed by the FUSE satellite during total eclipse and at three phases during chromospheric eclipse. We present the coadded, calibrated spectra. Download Citation | Observing and Analyzing the ζ Aurigae Systems | This chapter reviews the scientific information that has been extracted from the ζ Aur binaries by various methods, surveys.

Nov 5, - results relating to these species will be reviewed for H I1 regions. Savage, B.D., Fitzpatrick, E.L. This banner text can have markup. web; books; video; audio; software; images; Toggle navigation.

Full text of "Smithsonian year supplement: chronology and appendices" See other formats. Using Konigsberg's Fraunhofer heliometer, Bessel determined that 61 Cygni has a parallax of 0" (very close to the modern value of 0"), implying that the star was 10 l.y.

from Earth. The Royal Astronomical Society awarded him its Gold Medal for this achievement, which marked the first step towards accurately measuring stellar distances.

FUSE observations have been obtained during ingress and egress atmospheric eclipse phases, from a B-star height of RG*, until primary eclipse of the secondary star. Compared to a normal B9 V star, 22 Vul shows added wind absorption components in the B-star spectrum from the supergiant's wind at all phases.

Title: Publication Changes during the IAU History Authors: Abt, Helmut A. IAUSA Altcode: During the years of the International Astronomical Union, the worldwide astronomical publications have grown exponentially, converted almost entirely to English, and changed format from observatory publications to journals to online.

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annular eclipse The bright photosphere of the Sun can be seen surrounding the Moon during an annular eclipse. This eclipse was photographed on May 10 from Mexico. This content was uploaded by our users and we assume good faith they have the permission to share this book. If you own the copyright to this book and it is wrongfully on our website, we offer a simple DMCA procedure to remove your content from our site.

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