Week 1 Galactic Structure and Overview Flashcards

1
Q

what is the problem with baryonic matter in galaxies

A

it supplies inadequate mass to explain the dynamics of galaxies

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2
Q

what are 3 main things that the composition of an individual galaxy depends on

A

morphological type
mass
evolutionary age

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3
Q

define Population 1 stars

A

young ( < ~ 10^9 yr)
high luminosity and hot so appear blue
high level of enriched nucleosynthesised elements
typically found in disc and spiral galaxies

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4
Q

define Population 2 stars

A

old and massive
luminous but cold so appear red
metal poor
typically found in elliptical galaxies

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5
Q

how are stars classified

A

by a letter denoting temp and a roman numeral denoting luminosity
example: Sun is GV

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6
Q

define luminosity and its units

A

the intrinsic power output of the object, measured in W

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7
Q

define flux and its units

A

power received per unit area of detector measured in Wm^-2

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8
Q

define flux density and its units

A

flux per unit frequency range measured in units of Wm^-2Hz^-1

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9
Q

what does a higher magnitude basically tell us

A

higher positive magnitude means that the star is fainter

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10
Q

what is the apparent magnitude equation

A

m1 - m2 = -2.5 log [F1/F2]

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11
Q

what is the absolute magnitude equation

A

m - M = -5 + 5 log[d]

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