RV Tauri star | has period 1000 days (order of magnitude) | |
has definition A class of about 100 semiregular variable yellow supergiants of late spectral type (G-K), similar to W Virginis stars but with longer periods. Their spectra often contain emission lines, and their light curves have alternating deep and shallow minima. They have a large infrared flux. RVa stars maintain an approximately constant mean brightness; RVb stars have long-term (on the order of 1000 days) periodicity. | |
is a kind of semiregular variable | |
semiregular variable | has amplitude variable | |
late star | has spectral type cooler than G2 | |
variable | has name designated with - 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
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has observational problem some difficulty in distinguishing between various kinds | |
has observable variation time scale within a period of decades | |
has light curve | |
has optical brightness variation 0.2 magnitudes or greater | |
star | has star surface temperature | |
has V magnitude | |
has B magnitude | |
has U magnitude | |
has position on celestial sphere from the point of view of Earth | |
has parallax from the point of view of Earth's orbit | |
has proper motion | |
has radiation at surface which is diffused out from the hotter core | |
has energy source gravitational contraction and or fusion | |
has energy production which takes place primarily within the core | |
has surface density which depends on luminosity class | |
has surface temperature greater than 1000 Kelvin | |
has apparent magnitude | |
has absolute magnitude | |
has age | |
has catalog star catalog | |
has material hydrogen, helium | |
has velocity determined from proper motion and radial velocity | |
has mass greater than 0.08 the sun's mass | |
celestial body | has spectra | |
physical object | has location or center of gravity | |
has angular momentum | |
has momentum | |
has temperature | |
has volume | |
has extent | |