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AC Herculis, is an RV Tauri variable and spectroscopic binary star in the constellation of Hercules. It varies in brightness between apparent magnitudes 6.85 and 9.0. AC Her is an RVa star, meaning it is an RV Tauri variable whose maximum and minimum magnitudes do not slowly vary over hundreds of days. It also is a very clear example of a common type of RV Tauri light curve where the maximum following a deep minimum is brighter than the maximum following a shallow minimum. In each period of 75.46 days it has two maxima and two minima.

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rdf:type
rdfs:label
  • AC Herculis (en)
  • ヘルクレス座AC星 (ja)
  • AC Herculis (sv)
  • AC Геркулеса (ru)
rdfs:comment
  • ヘルクレス座AC星(ヘルクレスざACせい)は、ヘルクレス座の方向にある脈動変光星である。 (ja)
  • AC Геркулеса (лат. AC Herculis, HD 170756) — тройная звезда в созвездии Геркулеса на расстоянии приблизительно 4159 световых лет (около 1275 парсек) от Солнца. Видимая звёздная величина звезды — от +9m до +6,85m. (ru)
  • AC Herculis, is an RV Tauri variable and spectroscopic binary star in the constellation of Hercules. It varies in brightness between apparent magnitudes 6.85 and 9.0. AC Her is an RVa star, meaning it is an RV Tauri variable whose maximum and minimum magnitudes do not slowly vary over hundreds of days. It also is a very clear example of a common type of RV Tauri light curve where the maximum following a deep minimum is brighter than the maximum following a shallow minimum. In each period of 75.46 days it has two maxima and two minima. (en)
foaf:name
  • AC Herculis (en)
foaf:depiction
  • http://commons.wikimedia.org/wiki/Special:FilePath/AC_Herculis_light_curve.png
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axis unitless
appmag v
b-v
  • +0.52 - +1.09 (en)
class
  • F2pIb-K4e (en)
component
  • A (en)
  • B (en)
constell
eccentricity
epoch
equinox
  • J2000.0 (en)
gravity
inclination
luminosity
mass
metal fe
  • −1.5 (en)
p error
parallax
period unitless
prop mo dec
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