The period ratio distribution of Kepler's candidate multiplanet systems

The mass ratio distribution of short period double degenerate stars

Short period double degenerates (DDs) are close white dwarf –white dwarf binary stars which are the result of the evolution of interacting binary stars. We present the first definitive measurements of the mass ratio for two DDs, WD0136+768 and WD1204+450, and an improved measurement of the mass ratio for WD0957−666. We compare the properties of the 6 known DDs with measured mass ratios to the p...

coordination of protective schemes in distribution and subtransmission systems including distributed generation

نصب منابع پراکنده در سیستم های توزیع و فوق توزیع علاوه بر مزیت های فراوان، مشکلاتی را هم به همراه دارد. یکی از این مشکلات تأثیر این منابع روی اندازه جریان های اتصال کوتاه است. به طور معمول از حفاظت های مبتنی بر اصل جریان زیاد در سیستم های توزیع و فوق توزیع استفاده می شود. از مهمترین طرح های حفاظتی استفاده شده در فیدرهای توزیع، حفاظت فیوز- ریکلوزر است. همچنین از طرح های حفاظتی جریان زیاد جهتی در...

Low Stellar Obliquities in Compact Multiplanet Systems

We measure the sky-projected stellar obliquities (λ) in the multiple-transiting planetary systems KOI-94 and Kepler-25, using the Rossiter-McLaughlin effect. In both cases the host stars are well-aligned with the orbital planes of the planets. For KOI-94 we find λ = −11±11◦, confirming a recent result by Hirano and coworkers. Kepler-25 was a more challenging case because the transit depth is un...

What to Expect from Transiting Multiplanet Systems

So far radial velocity (RV) measurements have discovered ∼ 25 stars to host multiple planets. The statistics imply that many of the known hosts of transiting planets should have additional planets, yet none have been solidly detected. They will be soon, via complementary search methods of RV, transit-time variations (TTV) of the known planet, and transits of the additional planet. When they are...

An Evaluation of the Systems Reliability Using Fuzzy Lifetime Distribution