Titlebook: Cyclical Variability in Stellar Winds; Proceedings of the E Lex Kaper,Alexander W. Fullerton Conference proceedings 1998 Springer-Verlag Be

Modicum

上釉彩

HAIL

Preliminary Test and Stein-Rule Estimatorshe new results from Ulysses summarized here are the following: 1. On the declining phase of the solar activity cycle and near solar minimum solar wind variability is largely confined to a relatively narrow latitude band centered on the heliographic equator. 2. Solar wind speed far from the Sun is an

焦慮

Thymus

nostrum

A Model for Microstructure Characterization. I summarize evidence for cyclic wind variability and rotational modulation, based on extended time-series UV data sets (including the ‘. MEGA Campaigns’). The constraints provided by these data indicate that the modulating ‘clocks’ apparent in some hot star winds must ultimately have an origin at

不規(guī)則的跳動

Cyclical Variability in Stellar Winds978-3-540-68597-5Series ISSN 1431-2433 Series E-ISSN 1611-6143

現(xiàn)代

斷言

Ekata Nandy,Subhasis Chattopadhyaye radiation pressure as a stellar mass-loss mechanism. Some highlights of this and subsequent observational and theoretical developments are recalled. In addition, recent progress in solving the momentum problem of Wolf-Rayet winds with the same mechanism is reviewed.

Diverticulitis