DOI: 10.1007/978-94-011-0147-9_53
关键词: Radiation pressure 、 Astronomy 、 Outflow 、 Stars 、 Photometry (optics) 、 Loss rate 、 Astrophysics 、 Physics 、 Linear relation
摘要: The relation between mass loss rate and pulsation period in carbon Miras is discussed. dust very low (about 2 x 10-10M⊙/yr) up to about P = 380 days, where there a sudden increase. For P> 400 days linear log M P. change the near may be related radiation pressure on becoming effective driving outflow.