<--- Back to Details
First PageDocument Content
Space / Star / Luminosity / Eddington luminosity / Sun / Main sequence / Limb darkening / Temperature / Jeans instability / Physics / Astronomy / Astrophysics
Date: 2014-05-12 00:06:46
Space
Star
Luminosity
Eddington luminosity
Sun
Main sequence
Limb darkening
Temperature
Jeans instability
Physics
Astronomy
Astrophysics

PhD Qualifying Exam (2010) --- 星球天文物理 What is limb darkening? Can the limb darkening be seen if the star were isothermal, that is, the temperature is a constant all over the star? Why? Finally, explain how t

Add to Reading List

Source URL: www.astro.ncu.edu.tw

Download Document from Source Website

File Size: 88,50 KB

Share Document on Facebook

Similar Documents

Cumulative emissions of CO2 and future non-CO2 radiative forcing determine the probability of limiting warming to 1.5°C a) Observed global temperature change and modeled responses to stylized anthropogenic emission and

Cumulative emissions of CO2 and future non-CO2 radiative forcing determine the probability of limiting warming to 1.5°C a) Observed global temperature change and modeled responses to stylized anthropogenic emission and

DocID: 1xUk6 - View Document

Cumulative emissions of CO2 and future non-CO2 radiative forcing determine the probability of limiting warming to 1.5°C a) Observed global temperature change and modeled responses to stylized anthropogenic emission and

Cumulative emissions of CO2 and future non-CO2 radiative forcing determine the probability of limiting warming to 1.5°C a) Observed global temperature change and modeled responses to stylized anthropogenic emission and

DocID: 1xUiD - View Document

MODsense TM  An integrated and secure temperature monitoring solution. Qualified for monitoring medicinal product distribution.

MODsense TM An integrated and secure temperature monitoring solution. Qualified for monitoring medicinal product distribution.

DocID: 1xU1W - View Document

Cumulative emissions of CO2 and future non-CO2 radiative forcing determine the probability of limiting warming to 1.5°C a) Observed global temperature change and modeled responses to stylized anthropogenic emission and

Cumulative emissions of CO2 and future non-CO2 radiative forcing determine the probability of limiting warming to 1.5°C a) Observed global temperature change and modeled responses to stylized anthropogenic emission and

DocID: 1xTLF - View Document

Homework Download the House Insulation data – note that this is a text file. Regress gas consumption on the temperature.

DocID: 1xTkq - View Document