SV Vulpeculae is a classical Cepheid (δ Cepheid) variable star in the constellation Vulpecula. It is a supergiant at a distance of 8,700 light years....
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subgiant evolution is very rapid and it is difficult to detect examples. SV Vulpeculae has been proposed as a subgiant on its first crossing but was subsequently...
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few Cepheids with longer periods, including RS Puppis, SV Vulpeculae, and the unusual S Vulpeculae. The brightness variation in U Car is caused by fundamental...
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Berdnikov, L. N. (2004). "On the crossing mode of the long-period Cepheid SV Vulpeculae". Astronomy and Astrophysics. 423: 335–340. Bibcode:2004A&A...423..335T...
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HD 189733 b (redirect from V452 Vulpeculae b)
747L..20M. doi:10.1088/2041-8205/747/2/L20. S2CID 118492172. Berdyugina, S.V.; Berdyugin, A.V.; Fluri, D.M.; Piirola, V. (2011). "Polarized reflected...
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1938). Named after A. David Andrews. Anthelm's Nova/Star is Nova 1670 Vulpeculae, observed by Anthelme Voituret (aka père Anthelme / don Anthelme). Argelander's...
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"Dynamics of the circumstellar gas in the Herbig Ae stars BF Orionis, SV Cephei, WW Vulpeculae and XY Persei". Astronomy & Astrophysics. 419: 225–240. arXiv:astro-ph/0402614...
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