HR 5171, also known as V766 Centauri, is a yellow hypergiant in the constellation Centaurus. It is said to be either an extreme red supergiant (RSG) or...
28 KB (3,370 words) - 17:02, 3 December 2024
system to the Solar System, its neighbour in the sky Beta Centauri, and HR 5171, one of the largest stars yet discovered. The constellation also contains...
23 KB (2,825 words) - 19:50, 10 August 2024
System body), two asteroids gravitating toward each other until they touch. HR 5171, a yellow hypergiant previously thought to be a contact binary. Interacting...
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"VLTI/AMBER spectro-interferometry of the late-type supergiants V766 Cen (=HR 5171 A), σ Oph, BM Sco, and HD 206859". Astronomy & Astrophysics. 597: A9. arXiv:1610...
40 KB (4,527 words) - 02:08, 3 December 2024
further supports the binary nature of WOH G64. The interacting binary system HR 5171 is considered an analog to WOH G64, as it also contains a yellow hypergiant...
21 KB (2,290 words) - 04:15, 9 December 2024
supergiants (e.g. Zeta Cephei), or even as yellow (e.g. yellow hypergiant HR 5171 Aa).[citation needed] Red supergiants are cool and large. They have spectral...
34 KB (4,286 words) - 07:41, 14 December 2024
Centauri R Puppis IRC+10420 (V1302 Aql) IRAS 18357-0604 V766 Centauri (= HR 5171A) HD 179821 IRAS 17163-3907 V382 Carinae RSGC1-F15 V810 Centauri VdBH...
33 KB (3,828 words) - 14:04, 2 December 2024
MYSTIC 2022 Hypergiant star currently undergoing a great dimming event HR 5171 Aa 4.1±0.8 1060–1160 11740±1630 Very Large Telescope – VLTI/PIONIER 2014...
27 KB (1,613 words) - 03:49, 9 December 2024
eclipsing binaries are Epsilon Aurigae (Almaaz), VV Cephei, and V766 Centauri (HR 5171). Angular diameter measurements can be inconsistent because the boundary...
250 KB (10,635 words) - 08:02, 21 December 2024
Among other discoveries, Olivier Chesneau discovered the "peanut star" HR 5171, the fact that novae explode with an hourglass shape already a few days...
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Epsilon Aurigae (redirect from HR 1605)
larger component, at 1,280 R☉ for the yellow supergiant (comparable to HR 5171, a candidate for the largest known yellow hypergiant star), and 512 R☉...
34 KB (3,599 words) - 17:06, 18 September 2024
similar cool massive stars that have undergone one or more dimming events HR 5171, a similar star WOH G64 UY Scuti Westerlund 1 W26 The exact year of the...
32 KB (3,411 words) - 07:08, 18 September 2024
"VLTI/AMBER spectro-interferometry of the late-type supergiants V766 Cen (=HR 5171 A), σ Oph, BM Sco, and HD 206859", Astronomy & Astrophysics, 597: 16, arXiv:1610...
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Warren, P. R. (1973). "A model atmosphere analysis of the super-supergiant HR 5171". Monthly Notices of the Royal Astronomical Society. 161 (4): 427–444....
17 KB (1,597 words) - 12:34, 22 December 2024
1987 EH Sissons March 3, 1987 Anderson Mesa E. Bowell EOS 11 km MPC · JPL 5171 Augustesen 1987 SQ3 Augustesen September 25, 1987 Brorfelde P. Jensen slow...
232 KB (302 words) - 00:51, 26 November 2024
average distance between Saturn and the Sun 1.47 Tm – 9.9 au – diameter of HR 5171 A, a yellow hypergiant star. 1.5 Tm – 10 au – estimated diameter of VV...
188 KB (17,850 words) - 06:04, 19 December 2024
1943), friend of Edward Bowell who discovered this minor planet MPC · 5170 5171 Augustesen 1987 SQ3 Karl A. Augustesen (born 1945) has for several decades...
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1411 (category CS1 Croatian-language sources (hr))
1127–1128 Discordian calendar 2577 Ethiopian calendar 1403–1404 Hebrew calendar 5171–5172 Hindu calendars - Vikram Samvat 1467–1468 - Shaka Samvat 1332–1333...
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HPSE HGNC:5164 Q9Y251 7245 HPSE2 HGNC:18374 Q8WWQ2 7246 HPX HGNC:5171 P02790 7247 HR HGNC:5172 O43593 7248 HRAS HGNC:5173 P01112 7249 HRC HGNC:5178 P23327...
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National Academy of Sciences of the United States of America. 93 (10): 5166–5171. Bibcode:1996PNAS...93.5166E. doi:10.1073/pnas.93.10.5166. PMC 39426. PMID 8643547...
54 KB (5,178 words) - 18:43, 13 December 2024
Neher, R.; Riniker, B.; et al. (1968). "Human Calcitonin". Nature. 220 (5171): 984–986. Bibcode:1968Natur.220..984N. doi:10.1038/220984a0. ISSN 0028-0836...
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9:59:37 12:31:19 [26] 09220 129 27 1820 Mar 29 18:42:43 Partial -0.7112 0.5171 330.0 162.4 15:57:43 21:27:43 17:21:31 20:03:55 [27] 09266 129 28 1838 Apr 10...
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