Lecture 9 - Interstellar dust Flashcards

1
Q

What are dark clouds?

A

Absence of stars on photographic plates

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2
Q

What is interstellar reddening?

A

More extinction of blue light than red light, due to interstellar dust

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3
Q

What is a reflection nebula?

A

A cloud of interstellar dust visible by scattering from starlight

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4
Q

What is diffuse galactic light?

A

Light from an entire galaxy working as a reflection nebula

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5
Q

What are some evidence for interstellar dust?

A

Dark clouds, Interstellar extinction and reddening, polarization of starlight, reflection nebulae, diffuse galactic light,
continuum IR emission from clouds, microwave emission from clouds, X-ray halos around point sources

Interstellar depletions, existence of H2 in large amounts in ISM, Interstellar grains entering the solar system today, explains heating of diffuse ISM gas

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6
Q

What is R_V in the Milky Way?

A

About 3.1

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7
Q

How does a small R_V affect the extinction curve?

A

It becomes steep

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8
Q

How does a large R_V affect the extinction curve?

A

It becomes flat

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9
Q

Thermal spikes following photon absorptions are important for…

A

small particles (a<60Å)

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10
Q

PAH molecules consists of __ and __ atoms and are arranged like ____ .

A

hydrogen, carbon, hexagons

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11
Q

For what particle sizes are Rayleigh scattering relevant?

A

Particle < lambda/10

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12
Q

For what particle sizes are Mie scattering relevant?

A

1/10< Paricle/lambda< 1

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13
Q

For what particle sizes are Optical scattering relevant?

A

lambda < Particle

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14
Q

Mie theory is a classical scattering theory using series expansion in powers of what?

A

x=2pia/lambda

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15
Q

Extinction is the sum of ___ and ___ .

A

scattering, absorption

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16
Q

50% of interstellar grain mass are of order…

A

0.08<a></a>