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Author Question: How is dust usually observed around young protostars in stages 4-6? What will be an ideal ... (Read 50 times)

tfester

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on: Jul 27, 2018
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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Reply #1 on: Jul 27, 2018
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
Thanks for the timely response, appreciate it

carojassy25

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Reply 3 on: Yesterday
Excellent

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