1 - Introduction to galaxies Flashcards

1
Q

Define a galaxy

A

A large collection of starts, hot/cold gas and dust held together by mutual gravitation

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2
Q

What is the range of mass and size of all galaxies?

A

Mass - 10^6 - 10^13 solar masses
Size - 1-200+ kpc

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3
Q

What are the 5 types of galaxies?

A

Spirals, ellipticals, lenticulars, irregulars and peculiars

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4
Q

What size is an elliptical galaxy?

A

1-250 kpc

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5
Q

What size is a spiral galaxy?

A

1-100 kpc

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6
Q

What types of small galaxies are there?

A
  • Dwarf ellipticals (dE), 1-3kpc
  • Dwarf spheroidals (dSph), 0.1-0.5kpc
  • Dwarf irregulars (dI), <3kpc
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7
Q

What is the largest type of galaxy?

A
  • Giant ellipticals (cD), found in centre of clusters, absorb other galaxies, large diffused haloes
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8
Q

Define extrinsic and intrinsic properties

A
  • Extrinsic - properties that are observer-dependent or otherwise determined by external factors
  • Intrinsic - properties that are an integral property of the galaxy
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9
Q

Give examples of extrinsic properties of galaxies

A
  • Position in the sky
  • Apparent magnitude
  • Inclination angle
  • Distance
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10
Q

Give examples of intrinsic properties of galaxies

A
  • Physical size
  • Absolute magnitude
  • Rotation rate
  • Mass
  • Luminosity
  • Spatial characteristics
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11
Q

What are the two main catalogues of galaxies?

A

1780 Messier ~100 objects
New General Catalogue - 7800 objects

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12
Q

How have modern-day galaxy surveys improved?

A
  • Improved technology e.g - CCD detectors
  • Modern-day computing power allows us to sift and analyse vast amount of data
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13
Q

What is the SDSS?

A

Sloan digital sky survey:
- Surveying 1/4 of sky
- 10^6 galaxies
- ~1000Mpc

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14
Q

What is the dark energy survey?

A

DES:
Used 4m optical telescope equipped with 570 mega-pixel camera to survey ~300 million galaxies in 5 optical filters

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15
Q

Name 2 radio surveys

A
  • FIRST - ~9000 deg^2, 800
    000 sources
  • NVSS - ~34000 deg^2 (82% of
    sky), 1.8 million sources
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16
Q

Name 3 infrared surveys

A
  • IRAS - 350000, ~11000 galaxies
  • 2MASS - near-IR, all sky
  • SPITZER - SWIPE survey
    covering 50 deg^2, ~2 million
    galaxies
17
Q

What are 2 future galaxy survey projects?

A
  • Vera Rubin Telescope - 10 million
    galaxies surveyed over full
    hemisphere of sky every 3 nights,
    sensitive to transient sources
  • SKA - array of linked dishes and
    antennae across 1000s of km, will
    map hydrogen emission from over
    a billion galaxies
18
Q

What data issues do galaxy surveys produce?

A

Generate petabyte levels of data, in huge archives such as NASA Extragalactic Database (NED), suitable currently but datasets rapidly growing

19
Q

What is citizen science?

A

Solution to data issues, Example was galaxy zoo - public sift through and classify galaxies from SDSS
Distributed computing clients such as BOINC - allows PC users to analyse data with screensaver programs

20
Q

What is the Hubble Deep Field?

A
  • Unique survey
  • Several degrees away from any
    bright star, field devoid of amy
    a nearby bright objects/sources
  • Field has low IR cirrus flux from
    dust
  • Low extinction (from dust), low
    hydrogen column density