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Author Question: How is dust usually observed around young protostars in stages 4-6? What will be an ideal ... (Read 89 times)

tfester

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How is dust usually observed around young protostars in stages 4-6?
 
  What will be an ideal response?

Question 2

What stage of star formation is the zero-age main sequence?
 
  What will be an ideal response?



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trog

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Answer to Question 1

As the nebula contracts, it forms a dusty disk around the protostar's equator; often these are seen in profile with HST images around the protostars.

Answer to Question 2

At stage 7, the zero-age main-sequence star is fusing hydrogen and on the main sequence, to stay there for as long as it has sufficient hydrogen to remain stable.




tfester

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Reply 2 on: Jul 27, 2018
Great answer, keep it coming :)


zacnyjessica

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Reply 3 on: Yesterday
Thanks for the timely response, appreciate it

 

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