Gamma Cassiopeiae oor Spaans
Gamma Cassiopeiae
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Gamma Cassiopeiae
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Gamma Cassiopeiae became Navi – Ivan (Gus Grissom's middle name) spelled backwards.
He tenido pesadillas en donde lo veoWikiMatrix WikiMatrix
Its apparent magnitude is +5.4 and it is classified as a Gamma Cassiopeiae type variable star.
NB: Los totales pueden presentar diferencias debidas al redondeoWikiMatrix WikiMatrix
Classed as a Gamma Cassiopeiae variable or shell star, it is of spectral type B2II-IIIe and lies around 1430 light years distant from Earth.
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The 5th magnitude stars are all variables: one (NV Puppis) is a Gamma Cassiopeiae variable, and the other (NW Puppis) is a Beta Cephei variable.
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Gamma Cassiopeiae is the prototype of a small group of stellar sources of X-ray radiation that is about 10 times stronger than emitted from other B or Be stars.
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The class is named after the prototype star, gamma Cassiopeiae, which underwent a famous outburst back in 1937.
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It is the prototype of the class of Gamma Cassiopeiae variable stars.
Un ensayo psicológicoParaCrawl Corpus ParaCrawl Corpus
Emission-line stars, such as Gamma Cassiopeiae and Sheliak, which are in modern class Be.
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Gamma Cassiopeiae A, the bright primary, is itself a spectroscopic binary with an orbital period of about 203.5 days and an eccentricity alternately reported as 0.26 and "near zero."
¿ Les mentiste?ParaCrawl Corpus ParaCrawl Corpus
Also known as the ghost of Cassiopeia, IC 63 is being shaped by radiation from a nearby unpredictably variable star, Gamma Cassiopeiae, which is slowly eroding away the ghostly cloud of dust and gas.
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The question how the discs around active stars known as Be-stars rotate was posed since the discovery of the first one, Gamma Cassiopeiae, by Italian astronomer Father Angelo Secchi, exactly 140 years ago, on 23 August 1866 in Rome.
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11 sinne gevind in 4 ms. Hulle kom uit baie bronne en word nie nagegaan nie.