Transient Mass-loss Analysis of Solar Observations Using Stellar Methods

Conference Summary: Mass Loss from Stellar Clusters

Mass loss at the lowest stellar masses ⋆

We report the discovery of a jet in a [SII] image of Par-Lup3-4, a remarkable M5-type pre-main sequence object in the Lupus 3 star-forming cloud. The spectrum of this star is dominated by the emission lines commonly interpreted as tracers of accretion and outflows. Par-Lup3-4 is therefore at the very low-mass end of the exciting sources of jets. High resolution spectroscopy shows that the [SII]...

analysis of ruin probability for insurance companies using markov chain

در این پایان نامه نشان داده ایم که چگونه می توان مدل ریسک بیمه ای اسپیرر اندرسون را به کمک زنجیره های مارکوف تعریف کرد. سپس به کمک روش های آنالیز ماتریسی احتمال برشکستگی ، میزان مازاد در هنگام برشکستگی و میزان کسری بودجه در زمان وقوع برشکستگی را محاسبه کرده ایم. هدف ما در این پایان نامه بسیار محاسباتی و کاربردی تر از روش های است که در گذشته برای محاسبه این احتمال ارائه شده است. در ابتدا ما نشا...

Solar and Stellar Gamma Ray Observations with COMPTON

Observations by the Compton GRO are providing fundamental insights into the high-energy physics of solar ares. Most of the analyses have been made of the ares emitted by active region number 6659 in 1991 June. Hard X-ray pulses in ares show energy dependent delays of up to 200 ms due to time of ight, consistent with the location of an acceleration region above the soft X-ray loop and an impact ...

The Hipparcos observations and the mass of sub-stellar objects

The Hipparcos Intermediate Astrometric Data have been used lately to estimate the inclination of the orbital plane of candidate extrasolar planets. Whereas most of these investigations derive almost face-on orbits, we show that the astrometric data are seldom precise enough to undertake such studies and that the ‘face-on’ result might be just a spurious effect of the