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Type of variable star
this class is 56 Arietis, which bears the variable star designation SX Arietis. The following list contains selected SX Arietis variable that are of interest
SX_Arietis_variable
Zodiac constellation in the northern hemisphere
Hamal (Alpha Arietis, second magnitude), Sheratan (Beta Arietis, third magnitude), Mesarthim (Gamma Arietis, fourth magnitude), and 41 Arietis (also fourth
Aries_(constellation)
Star in the constellation Aries
Arietis is a single, variable star in the northern zodiac constellation of Aries. It has the variable star designation SX Arietis, while 56 Arietis is
56_Arietis
Variable star in the constellation Eridanus
visible to the naked eye of an observer far from city lights. It is a variable star, whose brightness varies slightly from 5.70 to 5.84 during its 1.374
HD_28843
Five-star system in the constellation Orion
variability of that star. Component E is an unusual variable star, classified as an SX Arietis variable and also known as V1030 Orionis. It is helium-rich
Sigma_Orionis
Star whose brightness fluctuates, as seen from Earth
of variable is named after the first Ap star to show rotationally-modulated photometric variability, Alpha2 Canum Venaticorum. SX Arietis variables These
Variable_star
Star in the constellation Scorpius
visible to the naked eye of an observer far from city lights. It is a variable star, whose brightness varies slightly from 5.40 to 5.47 during its 23
HD_142990
Variable star in the constellation Perseus
visible to the naked eye of an observer far from city lights. This is a variable star, whose brightness varies slightly from 5.45 to 5.53 during its 2.4761
HD_21699
Star in the southern constellation of Sculptor
Alpha Sculptoris is a B-type giant star. It is classified as an SX Arietis type variable star and its magnitude varies by less than a tenth of a magnitude
Alpha_Sculptoris
Star in the constellation Scorpius
no indications of long-term variability. In 1996 HR 5907 was given the variable star designation V1040 Scorpii. As of 2018, HR 5907 was the most luminous
HR_5907
Variable star in the constellation Orion
star with a stellar classification of B2V. It is classified as an SX Arietis variable that ranges in visual magnitude from 6.97 to 7.02 with a period of
V901_Orionis
Type of star
its helium spectral lines. Stars of this type are referred to as helium-variable. This is thought to occur when one hemisphere of the star's atmosphere
Helium-weak_star
B-type main-sequence star
vander Linden and Christiaan L. Sterken discovered that the star is a variable star, based on data obtained in 1984, and announced their discovery in
Sigma_Lupi
SX Areits variable; Corona Australis
166596; HR 6804; 3 G. CrA), or simply V692 CrA, is a whitish-blue hued variable star located in the southern constellation Corona Australis. It has a maximum
V692_Coronae_Australis
Variable star in the constellation Canis Major
Majoris is a variable star, in 1977. It was given its variable star designation in 1981. Samus et al. (2017) classify it as an SX Arietis variable that varies
12_Canis_Majoris
Binary star in the constellation Carina
Both stars appear to be deficient in helium. The primary is a helium variable star while the companion is a mercury-manganese star. The variability of
HD_90264
Ari) Designated φ Arietis by Johann Bode in his Uranographia Designated ξ1 Arietis by Johann Bode in his Uranographia Designated B Arietis by Johann Bode
List_of_stars_in_Aries
Binary star system in the constellation Orion
being an eclipsing binary or rotating ellipsoidal variable, and the primary is also am SX Arietis variable. The primary is a helium-strong, magnetic chemically
HD_37017
Variable star in the constellation Lupus
visible to the naked eye of an observer far from city lights. It is an SX Arietis variable star, varying from magnitude 5.76 to 5.81 over a period of 21.0594
HD_133880
Magnetic field generated inside a star
Intermediate polar Magnetic field Chemically peculiar star Polar (star) SX Arietis variable Vaughan–Preston gap Brainerd, Jerome James (July 6, 2005). "X-rays
Stellar_magnetic_field
Star in the constellation Lynx
broad, diffuse lines of helium. 36 Lyncis has been classified as an SX Arietis variable with an amplitude of 0.03 in visual magnitude and a rotationally-modulated
36_Lyncis
79158 45290 09h 13m 48.23s +43° 13′ 04.5″ 5.32 −0.90 573 B8IIIMNp SX Arietis variable, ΔV = 0.03m, P = 3.83 d 13 Lyn 13 48432 32489 06h 46m 49.49s +57° 10′ 09
List_of_stars_in_Lynx
Star in the constellation Centaurus
the strength of its neutral helium lines. It is classified as an SX Arietis type variable star and its brightness varies from magnitude +4.38 to +4.43 with
HD_125823
Star in the constellation Scorpius
in its surface brightness. It is classified as an SX Arietis variable, also known as helium variables. Their spectral lines also vary as the stars rotate
V957_Scorpii
Star in the constellation Puppis
since published research showing that k2 Puppis is the variable component. It is an SX Arietis variable with a period of 1.9093 days which is also the rotational
K_Puppis
Star in the constellation Cygnus
short-term variability with two or more periods, and is classified as an SX Arietis variable by Samus et al. (2017). It is spinning rapidly with a projected rotational
28_Cygni
Star in the constellation Auriga
the variability remains unknown. It may be a type of SX Arietis variable. It was given its variable star designation in 1972. HD 34626 has exhausted its
HD_34626
Constellation in the southern celestial hemisphere
apparent magnitude 6.5. The brightest star is Alpha Sculptoris, an SX Arietis-type variable star with a spectral type B7IIIp and an apparent magnitude of 4
Sculptor_(constellation)
Overview of the scientific field of astronomy
Alpha² Canum Venaticorum variable SX Arietis Pulsar Eclipsing binary Algol variable Beta Lyrae variable W Ursae Majoris variable Supernova Classes Type
Outline_of_astronomy
Type of variable star
to as rapidly oscillating α2 Canum Venaticorum variables. Both the roAp stars and some α2 CVn variables lie on the δ Scuti instability strip and are magnetic
Rapidly_oscillating_Ap_star
(celestial object) SX ARIetis, a class of rotating variable stars named after SX Arietis, the archetype for the class SXPHE – (celestial object) SX PhoEnicis,
List_of_astronomy_acronyms
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