Z Camelopardalis star Comparison Table

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physical object > natural object > celestial body > collection of stars > star system > binary star > close binary > nova > dwarf nova > Z Camelopardalis star

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Z Camelopardalis star comparison table

Subject has energy release has spectral type has reference is part of has extent has age has surface temperature has orbital period become has velocity is an instance of has surface density has optical brightness variation has star surface temperature has V magnitude has parallax has observational problem has light curve has position on celestial sphere has location has angular momentum has radiation at surface has acronym has B magnitude has temperature has abundance has prototype has recovery time has spectra has proper motion has amplitude has energy source has energy production has catalog has outburst start time has absolute magnitude has U magnitude has volume has momentum has peak brightness has apparent magnitude has material has mass has name designated with has observable variation time scale has emission line has use has synonym has definition has number of star

Z Camelopardalis 10⁴⁴ ergs Oppenheimer, B.D., Kenyon, S.J., Mattei, J.A.: 1998, AJ 115, 1175. An Analysis of AAVSO Observations of Z Camelopardalis Milky Way greater than 1000 Kelvin naked eye star determined from proper motion and radial velocity Z Camelopardalis star 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 AAVSO from the point of view of Earth or center of gravity which is diffused out from the hotter core Z Cam half the stars in the solar neighborhood are members of star systems Z Camelopardalis gravitational contraction and or fusion which takes place primarily within the core star catalog hydrogen, helium greater than 0.08 the sun's mass
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 nova peak brightness distance determination explosive variable is a dwarf nova with standstills in the light curve 2

Next dwarf nova: SS Cygni star Up: dwarf nova Previous dwarf nova: VW Hydri

Subject	has energy release	has spectral type	has reference	is part of	has extent	has age	has surface temperature	has orbital period	become	has velocity	is an instance of	has surface density	has optical brightness variation	has star surface temperature	has V magnitude	has parallax	has observational problem	has light curve	has position on celestial sphere	has location	has angular momentum	has radiation at surface	has acronym	has B magnitude	has temperature	has abundance	has prototype	has recovery time	has spectra	has proper motion	has amplitude	has energy source	has energy production	has catalog	has outburst start time	has absolute magnitude	has U magnitude	has volume	has momentum	has peak brightness	has apparent magnitude	has material	has mass	has name designated with	has observable variation time scale	has emission line	has use	has synonym	has definition	has number of star
Z Camelopardalis	10⁴⁴ ergs		Oppenheimer, B.D., Kenyon, S.J., Mattei, J.A.: 1998, AJ 115, 1175. An Analysis of AAVSO Observations of Z Camelopardalis	Milky Way			greater than 1000 Kelvin		naked eye star	determined from proper motion and radial velocity	Z Camelopardalis star	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 AAVSO	from the point of view of Earth	or center of gravity		which is diffused out from the hotter core	Z Cam			half the stars in the solar neighborhood are members of star systems	Z Camelopardalis					gravitational contraction and or fusion	which takes place primarily within the core	star catalog								hydrogen, helium	greater than 0.08 the sun's mass	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		nova peak brightness distance determination	explosive variable	is a dwarf nova with standstills in the light curve	2