flare star Comparison Table

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flare star comparison table

Subject has bolometric magnitude has spectral type is part of has orbital period is an instance of has parallax has eccentricity has radiu has distance has prototype has abundance has apparent magnitude has mass has emission line has synonym has definition has angular separation has number of star

Proxima Centauri M _bol = 11.66 dM4e Centaurus flare star 0'.765 R = 1.3 × 10¹⁰ cm 4.25 light-years 70 percent of all stars M = 0.1 M_sun UV Ceti star An flare star probably associated with the alpha Centauri system. It is the closest star to the Sun.

UV Ceti M6e V Cetus 26.5 years binary star from the point of view of Earth's orbit e = 0.615 2.8 pc UV Ceti half the stars in the solar neighborhood are members of star systems M_v = 15.3 and 15.8 0.15 M_sun hydrogen Luyten 726-8 B Late-type dwarf with spectra showing hydrogen emission lines. Faint flare star of very low mass. Like other flare stars, it is a member of a binary system in which both components are of nearly equal brightness. Radio flares have also been observed. 1".0 2

Wolf 359 M Leo flare star from the point of view of Earth's orbit 70 percent of all stars greater than 0.08 the sun's mass UV Ceti star A nearby flare star.

Subject	has bolometric magnitude	has spectral type	is part of	has orbital period	is an instance of	has parallax	has eccentricity	has radiu	has distance	has prototype	has abundance	has apparent magnitude	has mass	has emission line	has synonym	has definition	has angular separation	has number of star
Proxima Centauri	M _bol = 11.66	dM4e	Centaurus		flare star	0'.765		R = 1.3 × 10¹⁰ cm	4.25 light-years		70 percent of all stars		M = 0.1 M_sun		UV Ceti star	An flare star probably associated with the alpha Centauri system. It is the closest star to the Sun.
UV Ceti		M6e V	Cetus	26.5 years	binary star	from the point of view of Earth's orbit	e = 0.615		2.8 pc	UV Ceti	half the stars in the solar neighborhood are members of star systems	M_v = 15.3 and 15.8	0.15 M_sun	hydrogen	Luyten 726-8 B	Late-type dwarf with spectra showing hydrogen emission lines. Faint flare star of very low mass. Like other flare stars, it is a member of a binary system in which both components are of nearly equal brightness. Radio flares have also been observed.	1".0	2
Wolf 359		M	Leo		flare star	from the point of view of Earth's orbit					70 percent of all stars		greater than 0.08 the sun's mass		UV Ceti star	A nearby flare star.

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