Classification of intrinsic variables. IX. The Cepheid domain.
Abstract
Intermediate band, Hβ and RI observations have been obtained throughout the cycle of variation for 135 high mass, long-period and short-period cepheids (LPC and SPC). This material, together with the observations previously discussed for some 100 ultrashort periods cepheids (USPC), is used to delineate the cepheid domain in the (β,[C1]) and (MBol,log Te) planes. The independently derived luminosity calibrations for bright giants and supergiants previously published are found to closely reproduce the luminosities derived from the Sandage-Tammann PL relation for most variables. The theoretical "fundamental blue edge," computed by Iben and Tuggle with Y = 0.38, closely represents the blue edge of the cepheid domain.
- Publication:
-
The Astronomical Journal
- Pub Date:
- March 1983
- DOI:
- Bibcode:
- 1983AJ.....88..361E
- Keywords:
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- Astronomical Catalogs;
- Cepheid Variables;
- Giant Stars;
- Light Curve;
- Red Shift;
- Star Clusters;
- Stellar Color;
- Stellar Evolution;
- Stellar Luminosity;
- Supergiant Stars;
- Astronomy