Can stellar winds account for temperature fluctuations in HII regions?. The case of NGC 2363
We compare the rate of kinetic energy injected by stellar winds into the extragalactic H II region NGC 2363 to the luminosity needed to feed the observed temperature fluctuations. The kinetic luminosity associated to the winds is estimated by means of two different evolutionary synthesis codes, one of which takes into account the statistical
Luridiana, V. et al.
Fecha de publicación:
12
2001