Multiple Choice
The H-R diagram main-sequence of stars has a limit at the lower-mass or energy-output end because
A) low-mass stars form from the interstellar medium very rarely.
B) low-mass objects are composed primarily of solids, not gases.
C) pressure does not depend on temperature in degenerate matter.
D) the lower limit represents when the radius of the star would be zero.
E) there is a minimum temperature for hydrogen nuclear fusion (the definition of a star) .
Correct Answer:

Verified
Correct Answer:
Verified
Q80: There is a main-sequence mass-luminosity relation because<br>A)helium
Q81: T Tauri stars are in hydrostatic equilibrium.
Q82: The Sun has a core in which
Q83: What is the difference between the proton-proton
Q84: The interstellar medium is made of _
Q86: The CNO cycle requires higher temperatures than
Q87: What is the lifetime of a
Q88: Opacity is<br>A)the balance between the pressure and
Q89: The carbon-nitrogen-oxygen cycle<br>A)operates at a slightly lower
Q90: Star clusters are important to the study