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...

Hamal (Alpha Arietis, second magnitude), Sheratan (Beta Arietis, third magnitude), Mesarthim (Gamma Arietis, fourth magnitude), and 41 Arietis (also fourth...

A variable star is a star whose brightness as seen from Earth (its apparent magnitude) changes systematically with time. This variation may be caused by...

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...

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...

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...

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...

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...

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...

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...

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...

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...

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...

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...

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...

(celestial object) SX ARIetis, a class of rotating variable stars named after SX Arietis, the archetype for the class SXPHE – (celestial object) SX PhoEnicis,...

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...

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...

Intermediate polar Magnetic field Chemically peculiar star Polar (star) SX Arietis variable Vaughan–Preston gap Brainerd, Jerome James (July 6, 2005). "X-rays...

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...

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...

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...

II (ρ3 Ari), Al Buṭain III (ε Ari) and Al Buṭain IV (ζ Ari) SIMBAD, 50 Arietis (Retrieved 27 July 2012) Abt, Helmut A. (2008). "Visual Multiples. IX....

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...

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...

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...

V1046 Orionis was found to be a variable star by L. A. Balona in 1997, and is now classified as an SX Arietis variable. The star undergoes periodic changes...

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...

Alpha² Canum Venaticorum variable SX Arietis Pulsar Eclipsing binary Algol variable Beta Lyrae variable W Ursae Majoris variable Supernova Classes Type...

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...