| 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.
|
