How to answer this question, 21-cm emission line

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SUMMARY

The discussion centers on the limitations of 21-cm emission in determining the rotation curve of the Milky Way galaxy at galactocentric radii less than that of the Solar System. Participants express confusion regarding the question posed in a lab script, highlighting the need for clarity on whether "the Galaxy" refers specifically to the Milky Way. Key points include the geometric constraints that only allow stars closer to the galactic center than the Sun to be measured effectively, as they are the only ones moving directly towards or away from Earth.

PREREQUISITES
  • Understanding of 21-cm emission and its significance in astrophysics
  • Familiarity with the concept of galactocentric radii
  • Knowledge of the Milky Way galaxy's structure and rotation curves
  • Basic principles of radio astronomy and spectral lines
NEXT STEPS
  • Research the principles of 21-cm emission and its applications in galaxy rotation studies
  • Study the geometric relationships in galactic dynamics, particularly regarding star motion
  • Learn about the Milky Way's rotation curve and its implications for dark matter
  • Explore the techniques used in radio astronomy for measuring galactic structures
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Astronomy students, astrophysicists, and researchers interested in galactic dynamics and the application of radio astronomy in studying the Milky Way galaxy.

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TL;DR Summary: Completely clueless on how to answer this question, came up as part of an assessed lab script

Why does 21-cm emission only give the rotation curve of the Galaxy at galactocentric radii less than that of the Solar system?

The lab script asking this question made zero clarification on how to begin answering it, as have internet searches. Completely clueless.
 
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jqmhelios said:
TL;DR Summary: Completely clueless on how to answer this question, came up as part of an assessed lab script

Why does 21-cm emission only give the rotation curve of the Galaxy at galactocentric radii less than that of the Solar system?

The lab script asking this question made zero clarification on how to begin answering it, as have internet searches. Completely clueless.
Reading this, it sounds like there is context or language omitted from this question (possibly discernible from the overall total package and not the specific question) that is necessary to understand what is being asked.

For example, is "the Galaxy" the Milky Way galaxy, or any particular arbitrary galaxy that is being observed?

Which way is the radio-telescope pointed?
 
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jqmhelios said:
TL;DR Summary: Completely clueless on how to answer this question, came up as part of an assessed lab script

Why does 21-cm emission only give the rotation curve of the Galaxy at galactocentric radii less than that of the Solar system?

The lab script asking this question made zero clarification on how to begin answering it, as have internet searches. Completely clueless.
You need to provide more details...

Does that measurement test the speed of the stars?

Are spectral lines of hydrogen used?

Does the measurement only take place if the star is moving either straight towards us or straight away from us? ( Earth - Solar System)

If this above is the case, then it is a simple geometric problem.

Only stars that are closer to the galactic center than the Sun can be caught in position when they are moving straight towards us or straight away from us.

I need to draw this to explain...
galaxy_rotation_H_I_line.png

Only the stars that are on this circle move either straight towards us or straight away from us.
 
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