PHYS633 Introduction to Stellar Astrophysics                 Spring 2008

Homework 1: The Main Sequence Mass – Luminosity relation

Due in class on Monday, February 18th, 2008

The two files Astrometric_Binaries.txt and Eclipsing_Binaries.txt contain data from astrometric binaries and double line eclipsing binaries, respectively. The 1st column contains the name of the star, the 2nd column contains the absolute bolometric magnitude, MBol, and the 3rd column contains the mass in units of solar mass ( ).

(a)    Use the relation

                                                                              

to convert MBol to luminosity in units of solar luminosity ( ).

(b)   For each data set plot against .

(c)    By fitting a straight line to the combined data sets, determine the slope of the Mass-Luminosity relation, i.e. find α where the fitted line is

                                                                                

(d)   Identify the two stars in the astrometric binaries data set that deviate most from the straight line fit. What kind of stars are they?

[This homework is most easily done using software.  I have had success with the graphing software AXUM and the spread sheet software EXCEL.]