single line spectroscopic binary Comparison Table

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Next spectroscopic binary: Spica Up: spectroscopic binary Previous spectroscopic binary: Plaskett's star

single line spectroscopic binary comparison table

Subject has spectral type is part of has extent has age has surface temperature has orbital period is an instance of has velocity has surface density has optical brightness variation has star surface temperature has V magnitude has parallax has light curve has observational problem has position on celestial sphere has color has location has angular momentum has absorption line has radiation at surface has B magnitude has temperature has abundance has spectra has period has proper motion has amplitude has energy source has energy production has eclipse duration has catalog has absolute magnitude has wavelength has U magnitude has volume has momentum has apparent magnitude has material has mass has name designated with has observable variation time scale has synonym has luminosity class has number of star

Vela X-1 B0.5 Ib celestial sphere 11000 to 28000 K 8.96 days single line spectroscopic binary determined from proper motion and radial velocity which depends on luminosity class 0.2 magnitudes or greater from the point of view of Earth's orbit some difficulty in distinguishing between various kinds from the point of view of Earth blue-white or center of gravity He I which is diffused out from the hotter core half the stars in the solar neighborhood are members of star systems gravitational contraction and or fusion which takes place primarily within the core star catalog X-ray 7 hydrogen, helium of unseen companion 1.7 to 15 M_sun, with a probable value of about 2.6 M_sun.
R, S, T, U, V, W, X, Y, or Z and the genitive of the latin constellation name
RR, RS, RT, RU, RV, RW, RX, RY, or RZ and the genitive of the latin constellation name when the single letter designations are exhausted
AA...AZ, BB...BZ, etc. (omitting J), which ends with QQ...QZ and the genitive of the latin constellation namewhen the RR...RZ designations are exhausted
V 335, V 336, etc., when the double letter designations are exhausted
within a period of decades 3U 0900-40 I 2

Next spectroscopic binary: Spica Up: spectroscopic binary Previous spectroscopic binary: Plaskett's star

Subject	has spectral type	is part of	has extent	has age	has surface temperature	has orbital period	is an instance of	has velocity	has surface density	has optical brightness variation	has star surface temperature	has V magnitude	has parallax	has light curve	has observational problem	has position on celestial sphere	has color	has location	has angular momentum	has absorption line	has radiation at surface	has B magnitude	has temperature	has abundance	has spectra	has period	has proper motion	has amplitude	has energy source	has energy production	has eclipse duration	has catalog	has absolute magnitude	has wavelength	has U magnitude	has volume	has momentum	has apparent magnitude	has material	has mass	has name designated with	has observable variation time scale	has synonym	has luminosity class	has number of star
Vela X-1	B0.5 Ib	celestial sphere			11000 to 28000 K	8.96 days	single line spectroscopic binary	determined from proper motion and radial velocity	which depends on luminosity class	0.2 magnitudes or greater			from the point of view of Earth's orbit		some difficulty in distinguishing between various kinds	from the point of view of Earth	blue-white	or center of gravity		He I	which is diffused out from the hotter core			half the stars in the solar neighborhood are members of star systems					gravitational contraction and or fusion	which takes place primarily within the core		star catalog		X-ray				7	hydrogen, helium	of unseen companion 1.7 to 15 M_sun, with a probable value of about 2.6 M_sun.	R, S, T, U, V, W, X, Y, or Z and the genitive of the latin constellation name RR, RS, RT, RU, RV, RW, RX, RY, or RZ and the genitive of the latin constellation name when the single letter designations are exhausted AA...AZ, BB...BZ, etc. (omitting J), which ends with QQ...QZ and the genitive of the latin constellation namewhen the RR...RZ designations are exhausted V 335, V 336, etc., when the double letter designations are exhausted	within a period of decades	3U 0900-40	I	2