41. Epsilon Coronae Australis is an F4V dwarf star with an effective temperature of 6000 Kelvin. 42. Omicron 1 Eridani is an outer atmosphere at an effective temperature of 6, 963 K. 43. Only the nematic mesophase has thermochromic properties; this restricts the effective temperature range of the material. 44. Eta 1 Coronae Australis is an A3V dwarf star with an effective temperature of 9000 Kelvin. 45. In the case of stars with few observations, it must be computed assuming an effective temperature . 46. This is giving the star an outer atmosphere at an effective temperature of 11, 055 K. 47. Eta 2 Coronae Australis is a B9IV subgiant star with an effective temperature of 11000 Kelvin. 48. Gamma Coronae Australis A is an F8V dwarf star with an effective temperature of 5500 Kelvin. 49. Such electrons are characterized by high effective temperatures . 50. It is radiating this energy into space from its outer envelope at an effective temperature of.
