Anser, α Vul, 6 Vulpeculae, BD+24°3759, FK5 1508, HD 183439, HIP 95771, HR 7405, SAO 87261, CCDM J19288+2442A, WDS J19287+2440A[9]
Database references
SIMBAD
data
Alpha Vulpeculae (α Vulpeculae, abbreviated Alpha Vul, α Vul), officially named Anser/ˈænsər/,[10] is the brightest star in the constellation of Vulpecula. It is approximately 291 light-years from Earth. It forms a wide optical binary with 8 Vulpeculae.[11]
Alpha Vulpeculae is a red giant of spectral class M1 and has an apparent magnitude of +4.4. It has been analyzed as a member of the Arcturus stream, a group of stars with high proper motion and metal-poor properties thought to be the remnants of a small galaxy consumed by the Milky Way.[12]
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AlphaVulpeculae (α Vulpeculae, abbreviated Alpha Vul, α Vul), officially named Anser /ˈænsər/, is the brightest star in the constellation of Vulpecula...
magnitude in this constellation. The brightest star in Vulpecula is AlphaVulpeculae, a magnitude 4.44m red giant at an approximate distance of 291 light-years...
jet fighter project of the 1950s Anser, the proper name of the star AlphaVulpeculae Argonne–Northwestern Solar Energy Research Center Sega Mega Anser,...
include the red giant Kappa Gruis and the M-class stars 27 Cancri, AlphaVulpeculae and RT Hydrae. List of stellar streams Ibata, Rodrigo; Gibson, Brad...
8 Vulpeculae is star located about 457 light years away in the northern constellation of Vulpecula. It lies just 7′ from AlphaVulpeculae and the two...
ER Vulpeculae is a binary star system in the northern constellation of Vulpecula, abbreviated ER Vul. It is a variable star system with a brightness that...
than visible light. In March 2010, transit observations using HI Lyman-alpha found that this planet is evaporating at a rate of 1-100 gigagrams per second...
HD 192685, also known as QR Vulpeculae or HR 7739, is a Be star about 1,000 ly away in the Vulpecula constellation. It is visible to the naked eye. HD...
could also exist brown dwarfs that merged with white dwarfs. The nova CK Vulpeculae might be a result of such a white dwarf–brown dwarf merger. Substellar...
Gall and Inglis. p. 52 – via Internet Archive. Kaler, James B. "Menkar (Alpha Ceti)". Stars. University of Illinois. Archived from the original on 2012-05-31...
"photographs of the nebulæ M 31, h 44, and h 51 Andromedæ, and M 27 Vulpeculæ". Monthly Notices of the Royal Astronomical Society. 49 (2): 65–66. Bibcode:1888MNRAS...
(1990). "The size and shape of (2) Pallas from the 1983 occultation of 1 Vulpeculae". Astronomical Journal. 99: 1636–1662. Bibcode:1990AJ.....99.1636D. doi:10...
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...
with DAO spectrograms -- XX. The early a stars epsilon Serpentis, 29 Vulpeculae and sigma Aquarii". Monthly Notices of the Royal Astronomical Society...
useful supergiant stars can be occulted by the Moon, including Antares A (Alpha Scorpii A). Examples of eclipsing binaries are Epsilon Aurigae (Almaaz)...
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...
exocometary systems (Beta Pictoris, HR 10, 51 Ophiuchi, HR 2174, 49 Ceti, 5 Vulpeculae, 2 Andromedae, HD 21620, HD 42111, HD 110411, and more recently HD 172555)...
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