Are Pop III Stars Finally Detected in I Zw 18?

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In summary, the authors found stars so hot that their light contained the recombination UV from doubly ionized Helium. This indicated that the stars were very young and had not yet made metals, which ruled out older stars as the sources of the light. The lack of a stellar wind indicated that these were the first stars to form in the galaxy, and they may provide an opportunity to explore the origins of the universe.
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Chronos
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This paper; http://arxiv.org/abs/1504.02742, Population III Stars in I Zw 18, claims potentially conclusive evidence of detection of pop III stars.
 
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Thanks for sharing, Chronos! I'm looking forward to hearing more about this.
 
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That's interesting. These are, perhaps, the first stars formed.
They are distinguished by very low "metal" (absence of elements heavier than H and He)

The authors found stars so hot that their light contained the recombination UV from doubly ionized Helium.
Takes very high temperature to get both electrons off a helium atom.

And apparently these very hot bright massive stars did not show evidence of WIND.
Stellar wind is caused by radiation pressure of star's light on heavier elements ("metals") like Oxygen and Carbon.

So these stars were so young that they had not made metals, and they were so early that the galaxy they formed in did not have metals made by earlier stars. These were pristine first-type stars. So-called PopIII

The windlessness seems to have been the clincher---the fact that here were these extremely hot intense stars whose ATMOSPHERES apparently contained only H and He.

Really interesting paper! Thanks for sharing.
 
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marcus said:
That's interesting. These are, perhaps, the first stars formed.
They are distinguished by very low "metal" (absence of elements heavier than H and He)

The same kind of stars that were the first stars formed, surely. My understanding of Zw 18 is that it's still a very active star forming galaxy, and in any case, the first pop III stars will be long gone, even in a galaxy 18 Mpc away.

But hey, a good analogy is fantastic.
 
  • #5
Good point 18 x 3.26 is only 59 million LY. This is relatively near, these stars are practically our contemporaries . But they are the same TYPE as the first stars----analogous to them as you say.
 
  • #6
marcus said:
Good point 18 x 3.26 is only 59 million LY. This is relatively near, these stars are practically our contemporaries . But they are the same TYPE as the first stars----analogous to them as you say.

Right! And being basically on our doorstep, they are good candidates for investigation too!
 

Related to Are Pop III Stars Finally Detected in I Zw 18?

1. What are Pop III stars?

Pop III stars, also known as Population III stars, are the first generation of stars that formed in the universe. They are composed almost entirely of hydrogen and helium, with very little, if any, heavier elements. They are thought to have formed approximately 13.6 billion years ago, shortly after the Big Bang.

2. How are Pop III stars detected?

Pop III stars are detected through various methods, including spectroscopy, which measures the chemical composition of a star, and photometry, which measures the brightness of a star. Additionally, observations of the cosmic microwave background radiation can also provide evidence of the existence of Pop III stars.

3. Why are Pop III stars important?

Pop III stars are important because they are the first stars to have formed in the universe. Their formation and evolution played a crucial role in shaping the early universe and creating the conditions necessary for the formation of later generations of stars and galaxies. Additionally, studying Pop III stars can provide insights into the composition and evolution of the universe.

4. How do Pop III stars differ from other stars?

Pop III stars differ from other stars in several ways. They are composed almost entirely of hydrogen and helium, with very little, if any, heavier elements. They are also much larger and hotter than most stars, with temperatures reaching over 100,000 Kelvin. Additionally, Pop III stars have much shorter lifetimes, lasting only a few million years compared to billions of years for later generations of stars.

5. What impact do Pop III stars have on the universe?

Pop III stars have a significant impact on the universe. They played a crucial role in the formation of the first galaxies and in the production of heavier elements, which are necessary for the formation of planets and life. They also contribute to the reionization of the universe, the process of ionizing neutral gas and making it transparent to light. Pop III stars continue to have an impact on the universe today, as their remnants, such as black holes and neutron stars, can be observed in the modern universe.

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