K2-263 b: a 50 d period sub-Neptune with a mass measurement using HARPS-N

Evolutionary Analysis of Gaseous Sub-neptune-mass Planets with Mesa

Sub-Neptune-sized exoplanets represent the most common types of planets in the Milky Way, yet many of their properties are unknown. Here, we present a prescription to adapt the capabilities of the stellar evolution toolkit Modules for Experiments in Stellar Astrophysics (MESA) to model sub-Neptune mass planets with H/He envelopes. With the addition of routines treating the planet core luminosit...

Probabilistic Mass–radius Relationship for Sub-neptune-sized Planets

The Kepler Mission has discovered thousands of planets with radii <4 Å R , paving the way for the first statistical studies of the dynamics, formation, and evolution of these sub-Neptunes and super-Earths. Planetary masses are an important physical property for these studies, and yet the vast majority of Kepler planet candidates do not have theirs measured. A key concern is therefore how to map...

Using NSGA II Algorithm for a Three Objectives Redundancy Allocation Problem with k-out-of-n Sub-Systems

in the new production systems, finding a way to improving the product and system reliability in design is a very important. The reliability of the products and systems may improve using different methods. One of this methods is redundancy allocation problem. In this problem by adding redundant component to sub-systems under some constraints, the reliability improved. In this paper we worked on ...

Drawing k2, n: A lower bound

روابط بین رسته های ?/b,?/a,?/a و

در این پایان نامه ابتدا رسته ی کاما e/a، وابسته به رسته e را معرفی کرده ایم. سپس تابعگون هایی بین رسته های کامای e/a و e/b بدست آورده و نشان می دهیم این تابعگون ها زوج های الحاقی اند . همچنین موند مربوط به این زوج های الحاقی را ارائه خواهیم کرد. سرانجام با استفاده از تابعگون های بین رسته e/a و رسته کامای ریخت جزئی e/a روابطی بین رسته های فوق الذکر بدست می آوریم.