CO observations of the galaxy reveal
a. the location of dense neutral hydrogen clouds.
b. the location of population II stars.
c. the location of population I stars.
d. the location of the galactic corona.
e. the location of giant molecular clouds.
Question 2
If a star's spectrum does not contain spectral lines characteristic of a certain element, can we conclude that the star does not contain that element? Why or why not?
What will be an ideal response?