Week 2 Multi-Wavelength Night Sky, Effects of Dust & Blackbody radiation Flashcards

1
Q

give 3 general observations about the optical night sky

A

starfield dominates the detectable output
central bulge is obscured
some light comes from hot gas

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2
Q

give 2 general observations about the infrared night sky

A

less extinction in comparison to optical

cooler objects emit longer wavelength radiation

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3
Q

give 2 general observations about microwave night sky

A

CMBR is prevalent in background

most emission comes from thermal dust/gas

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4
Q

give 2 general observations about the radio night sky

A

emission not dependent on stars

most emission comes from B field

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5
Q

give 3 general observations about the X-ray night sky

A

general comes from supernova emission
has two obvious points source- AGN and Neutron stars
Extinction is present

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6
Q

give 3 general observations about gamma-ray night sky

A

no extinction present
two point sources of black hole and neutron stars
general emission resultant of annihilation reactions

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7
Q

what causes extinction

A

dust between a source and observer absorbing radiation

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8
Q

describe what happens to long and short wavelength radiation passing through dust

A

both becomes less intense however shorter wavelength is more likely to be scattered out of line of sight

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9
Q

what does extinction depend on

A

grain size

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10
Q

describe what extinction takes place for small, comparable and large grains

A

small - rayleigh scattering
comparable - mie scattering
large - extinction is independent of wavelength

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11
Q

what is true of thermal radiation spectrum

A

it is only temperature dependent

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12
Q

what does Kirchoffs law state

A

source function of a material in thermal eqm is equal to Planck function

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13
Q

how do you convert from wavelength Planck function to frequency Planck function

A

differentials

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