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12 Vulpeculae

12 Vulpeculae is a class B2.5V (blue main-sequence) star in the constellation Vulpecula. It is a variable Be star with an apparent magnitude varying from 4.78 to 4.97 and it is approximately 630 light years away based on parallax.

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Binocular Universe: Houston’s Triangle
The Coathanger, plotted as Brocchi's Cluster, is seen just above (north) of the "G" in Sagitta. From M27, look 2° due west to 5th-magnitude 12 Vulpeculae. Can you spot a faint glow just to the north? That’s the open cluster NGC 6830. Some two dozen ...
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5 Vulpeculae
It shines at magnitude +5.7/+8.1. Its celestial coordinates are RA 20 12.0 , dec +26° 29′. It surrounds the naked eye Be star 20 Vulpeculae , and is located near M27 (Dumbbell nebula), the nebula IC 4954 , and open clusters NGC 6882 and NGC 6940
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Photoelectric monitoring of bright Be stars. II - 1989, 1990, 1991
12 Vulpeculae, 28 Cygni, QR Vulpeculae, Omicron Andromedae, EW Lacertae, and KX Andromedae is reported and discussed. The nature and cause of the photometric variations and their relationship to variations at other wavelengths are explored.
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Photometric Monitoring of Bright Be Stars. IV. 1996-1999
We report long-term UBV observations of 15 bright, active Be stars, namely: X Persei, EW Canis Majoris, θ Coronae Borealis, 4 (V839) Herculis, 88 (V744) Herculis, 66 (V2048) Ophiuchi, NW Serpentis, CX Draconis, 12 (V395) Vulpeculae, 28 (V1624) Cygni ...
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The August 2016 Night Sky
The shower is spread over several weeks, reaching a sharp maximum between August 8 and 14 with a peak on 12 August. As the night unfolds ... on star charts but is still represented by Alpha Vulpeculae which is known as Anser or sometimes Lukida.
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X-Ray Spectroscopy of the Classical Nova V458 Vulpeculae with Suzaku (2008)
title = {X-Ray Spectroscopy of the Classical Nova V458 Vulpeculae with Suzaku ... equivalent extinction column density of ∼ 3 × 10 21 cm −2, a flux of ∼10 −12 erg s −1 cm −2, and a luminosity of ∼6×10 34 erg s −1 in the 0.3–3.0 ...
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Big Apple's Milky Way Galaxy: When Real Stars Shined Over NYC
The 5.4-magnitude star 24 Vulpeculae was readily seen without binoculars ... and he is also an on-camera meteorologist for News 12 Westchester, New York.
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SciTech Connect Journal Article: Isothermal dust condensation of Nova Vulpeculae 1976
Nova Vulpeculae 1976 has been followed with broad-band photometry at wavelengths of 0.5 to 12.5 microns from day 3 to day 235. Three definite phases are identified. They are expanding pseudophotosphere, free-free expansion, and dust condensation.
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The Little Fox
On most star charts Vulpecula, the Little Fox, seems to be nothing more than a formless splattering ... faint stars and does not include this constellation’s brightest, Alpha Vulpeculae. The average visual magnitude of the 12 stars that constitute ...
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Vulpecula - Wikipedia
Stars. There are no stars brighter than 4th magnitude in this constellation. The brightest star in Vulpecula is Alpha Vulpeculae, a magnitude 4.44 m red giant at a ...
en.wikipedia.org
Nova - Wikipedia
A nova (plural novae or novas) or classical nova (CN or plural CNe) is an astronomical event that causes the sudden appearance of a bright "new" star, that slowly ...
en.wikipedia.org
Lista di stelle - Wikipedia
Questa è una lista di stelle disposte in ordine alfabetico in base alla costellazione alla quale appartengono. Sono riportate solo le stelle a cui è stato dato un ...
it.wikipedia.org
全天88星座 一覧 - seiza-zukan.com
全天には88の星座がありますが、とびうお座やけんびきょう座など、日本からは見えないものもあります。下の一覧には89 ...
seiza-zukan.com
Stars
STARS With thanks to all, STARS celebrates over 3.9 million visitors! Happy Birthday: STARS, born January 30, 1998, is 19 years old! STARS has passed the 900 mark.
stars.astro.illinois.edu
Liste von Sternennamen – Wikipedia
Eigenname Bezeichnung; Baham, Biham: Theta Pegasi: Barnards Pfeilstern: Baten Kaitos: Zeta Ceti: Baten Algiedi: Omega Capricorni: Becrux / Mimosa: Beta Crucis: Beid
de.wikipedia.org
Список созвездий - edu.zelenogorsk.ru
01. Андромеда And Andromeda Andromedae 02. Близнецы Gem Gemini Geminorum 03.
edu.zelenogorsk.ru
Stjernebillede - Wikipedia, den frie encyklopædi
Stjernebillede kaldes hvert af de områder som nattehimlen er opdelt i. Stjernebilleder er et praktisk hjælpemiddel for astronomer når de ønsker at fortælle ...
da.wikipedia.org
Lijst van sterren - Wikipedia
Dit is een lijst van sterren die naast een aanduiding of catalogusnummer ook een traditionele naam hebben.
nl.wikipedia.org
Jan Heweliusz – Wikipedia, wolna encyklopedia
Jan Heweliusz, portret pędzla Daniela Schultza: Data i miejsce urodzenia: 28 stycznia 1611 Gdańsk, Rzeczpospolita Obojga Narodów: Data i miejsce śmierci
pl.wikipedia.org

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