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31 neue veränderliche Sterne

Astronomy and Astrophysics – Astronomy
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31.1907 Aurigae

Astronomy and Astrophysics – Astronomy
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31.4 day periodicity in Cyg X-3 ASM-data: evidence for a tertiary body or precessing disc ?

Astronomy and Astrophysics – Astronomy
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31.4- and 89.6-GHz flux density measurements of extragalactic radio sources

Astronomy and Astrophysics – Astronomy
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31.4-GHz flux density measurements of a complete sample of sources from the 5-GHz S5 survey

Astronomy and Astrophysics – Astronomy
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31.4-GHz flux density measurements of variable radio-sources.

Astronomy and Astrophysics – Astronomy
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316 neue Veränderlilche

Astronomy and Astrophysics – Astronomy
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318-MHz variability of complete samples of extragalactic radio sources

Astronomy and Astrophysics – Astronomy
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31st Annual Meeting of the American Astronomical Society (AAS) Solar Physics Division, Lake Tahoe, NV (USA), 18 - 22 Jun 2000. Abstracts of presented papers.

Astronomy and Astrophysics – Astronomy
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31st Meeting of the Division for Planetary Sciences of the American Astronomical Society

Astronomy and Astrophysics – Astronomy
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31st Meeting of the Division on Dynamical Astronomy of the American Astronomical Society

Astronomy and Astrophysics – Astronomy
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32 Cygni

Astronomy and Astrophysics – Astronomy
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32 GHz radio continuum observations of four shell-type supernova remnants

Astronomy and Astrophysics – Astronomy
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32 Meter Radio Telescopes in the Arabian Region

Astronomy and Astrophysics – Astronomy
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32-Channel Spectrophotometry of Stellar Flares

Astronomy and Astrophysics – Astronomy
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32-megapixel dual-color CCD imaging system

Astronomy and Astrophysics – Astronomy
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327 MHz observations of the galactic center: Possible detection of a deuterium absorption line.

Astronomy and Astrophysics – Astronomy
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327-MHz low noise front end.

Astronomy and Astrophysics – Astronomy
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32nd Meeting of the AAS Division on Dynamical Astronomy

Astronomy and Astrophysics – Astronomy
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32nd Meeting of the Division for Planetary Sciences of the American Astronomical Society

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