shell star Comparison Table

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shell star comparison table

Subject has companion is part of has orbital period is an instance of has abundance has primary has synonym has definition has number of star

17 Leporis M1 III Lepus binary star half the stars in the solar neighborhood are members of star systems A0 V A close binary system (A0 V, M1 III) with a shell-like spectrum indicating that mass transfer may be occurring from the late-type companion onto the A0 primary. 2

Pleione Taurus shell star 28 Tau A B8pe star, one of the brightest stars in the Pleiades, which developed an envelope or shell first observed in 1938. The shell increased in strength and attained its maximum intensity in 1945; thereafter it weakened and was scarcely visible by 1954. In 1972 it developed another shell. It is rotating so fast that it is unstable.

Subject	has companion	is part of	has orbital period	is an instance of	has abundance	has primary	has synonym	has definition	has number of star
17 Leporis	M1 III	Lepus		binary star	half the stars in the solar neighborhood are members of star systems	A0 V		A close binary system (A0 V, M1 III) with a shell-like spectrum indicating that mass transfer may be occurring from the late-type companion onto the A0 primary.	2
Pleione		Taurus		shell star			28 Tau	A B8pe star, one of the brightest stars in the Pleiades, which developed an envelope or shell first observed in 1938. The shell increased in strength and attained its maximum intensity in 1945; thereafter it weakened and was scarcely visible by 1954. In 1972 it developed another shell. It is rotating so fast that it is unstable.

Next emission line star: supernova Up: emission line star Previous emission line star: P Cygni star