Reasons why merging of spirals becomes red
by Ju Boo Lim - Sunday, 6 October 2019, 3:13 PM
Number of replies: 10
I think this is quite simple to explain
Since the spiral arms of galaxies are new with new blue and
hot population 1 stars, over time they slowly burn up their fuel and became
less hot and older. Their spectrum shifts from blue hot to the cooler red
colour
At the same time their spiral arms whatever their various
tunning fork classification, became to merge or coalesce, maybe I guess due to
the gravitational pull of their elliptical or oval centers which are more
massive due to the crowd of metal poor population 2 stars within their galactic nuclei.
When two spirals merging to form an elliptical galaxy they
began to contain older red stars.
These "centralized stars" are cooler, older and
redder than the metal rich population 1
blue and hotter stars
As the population 1 stars grow older and redder in the spirals,
they may merge to become ellipticals
Their centres too
became redder because they now contain larger content of old red stars
Older population 2 stars in the galactic nuclei are less rich in metal content than newer
population 1 stars in their spiral arms due to the blast of some massive stars
in supernovae spilling out their metal contents from nucleosynthesis outwards
to contaminate the gas clouds and dusts in the surroundings even before they
can form new less metal-rich
stars.
I think the shortest way to answer this question is, hot
blue spiral galaxies after merging they become older over time, and became
cooler and redder.
In reply to Ju Boo Lim
Re: Reasons why merging of spirals becomes red
by Dr. Grant Miller, University of Oxford
- Thursday, 10
October 2019, 5:06 PM
This is basically the right answer! Good work! The key is in
what you pointed out at the end. Red stars are cooler and older, so if merging
takes some time then those are the stars that will be left at the end, whereas
more of the younger, hotter blue stars from the original spiral galaxies will
have died off.
No comments:
Post a Comment