Galaxies & Cosmology (HEAC II) · Galaxies & Cosmology (HEAC II) 5 points, ht-2006 Teacher: Göran...

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Galaxies & Cosmology (HEAC II) 5 points, ht-2006 Teacher: Göran Östlin Lecture 8 Contents: - Active Galactic Nuclei - Galaxy formation theory

Transcript of Galaxies & Cosmology (HEAC II) · Galaxies & Cosmology (HEAC II) 5 points, ht-2006 Teacher: Göran...

Page 1: Galaxies & Cosmology (HEAC II) · Galaxies & Cosmology (HEAC II) 5 points, ht-2006 Teacher: Göran Östlin Lecture 8 Contents: - Active Galactic Nuclei - Galaxy formation theory.

Galaxies & Cosmology (HEAC II)5 points, ht-2006

Teacher: Göran Östlin

Lecture 8

Contents:- Active Galactic Nuclei

- Galaxy formation theory

Page 2: Galaxies & Cosmology (HEAC II) · Galaxies & Cosmology (HEAC II) 5 points, ht-2006 Teacher: Göran Östlin Lecture 8 Contents: - Active Galactic Nuclei - Galaxy formation theory.

Active galaxies / Active galactic nuclei (AGN)

Central enginevariability put limit on size: R ≤ c τvarSchwarzschild radius: Rs = 2 G M / c2

Rs = size approx Uranus orbit for 109 M

Accretion allows conversion of 0.1mc2

(fusion only 0.7%)Radiation pressure will larger than gravity if L > LEDD

Accretion disk very hot continuum source => X-raysBroad line region, dense ionised clouds, rapid movingNarrow line region, dilute ionised clouds, slower

reverbration mappingObscuring torus with dust and molecular gas,

sublimation evacuate central part -> torusRelativistic (superluminal) Jets, and radio Lobes

Page 3: Galaxies & Cosmology (HEAC II) · Galaxies & Cosmology (HEAC II) 5 points, ht-2006 Teacher: Göran Östlin Lecture 8 Contents: - Active Galactic Nuclei - Galaxy formation theory.
Page 4: Galaxies & Cosmology (HEAC II) · Galaxies & Cosmology (HEAC II) 5 points, ht-2006 Teacher: Göran Östlin Lecture 8 Contents: - Active Galactic Nuclei - Galaxy formation theory.

Unified AGN models

Idea: all AGN are basically the same phenomenaDiffering due to different viewing angle and scale:

Face on view: see all components: Sy1, QSO if looking into jet: Bl Lac (Blazar)

Edge on view: see only hot torus and NLR, Sy2

Why some radio loud while others not?

Unified BH model not perfect, but nothing else works

Page 5: Galaxies & Cosmology (HEAC II) · Galaxies & Cosmology (HEAC II) 5 points, ht-2006 Teacher: Göran Östlin Lecture 8 Contents: - Active Galactic Nuclei - Galaxy formation theory.

Unified Model

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Spiral seyfert2 with radio jets Seyfert1

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QSO evolution - where are they now?

Debate if fall off at z>3 is real

There must be many dead QSOs around in the local universe!

Page 8: Galaxies & Cosmology (HEAC II) · Galaxies & Cosmology (HEAC II) 5 points, ht-2006 Teacher: Göran Östlin Lecture 8 Contents: - Active Galactic Nuclei - Galaxy formation theory.

Kinematical evidence for BH in M87

+ Grav redshifted X-ray em-lines detected in Sy1’s

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Page 10: Galaxies & Cosmology (HEAC II) · Galaxies & Cosmology (HEAC II) 5 points, ht-2006 Teacher: Göran Östlin Lecture 8 Contents: - Active Galactic Nuclei - Galaxy formation theory.

Relation between black hole mass and sigma of host galaxy: a realtion between BH and Spheroid Mass-- Black Hole doesn’t care about disk-- Co-evolves with spheroid/bulge!

Page 11: Galaxies & Cosmology (HEAC II) · Galaxies & Cosmology (HEAC II) 5 points, ht-2006 Teacher: Göran Östlin Lecture 8 Contents: - Active Galactic Nuclei - Galaxy formation theory.

Intergalactic matterQSO used as lamps

Page 12: Galaxies & Cosmology (HEAC II) · Galaxies & Cosmology (HEAC II) 5 points, ht-2006 Teacher: Göran Östlin Lecture 8 Contents: - Active Galactic Nuclei - Galaxy formation theory.
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Metallicity vs redshift

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Metallicity vs ”scale”

Page 17: Galaxies & Cosmology (HEAC II) · Galaxies & Cosmology (HEAC II) 5 points, ht-2006 Teacher: Göran Östlin Lecture 8 Contents: - Active Galactic Nuclei - Galaxy formation theory.

Evolution of the neutral hydrogen density

Page 18: Galaxies & Cosmology (HEAC II) · Galaxies & Cosmology (HEAC II) 5 points, ht-2006 Teacher: Göran Östlin Lecture 8 Contents: - Active Galactic Nuclei - Galaxy formation theory.

Gunn-Peterson effect

Page 19: Galaxies & Cosmology (HEAC II) · Galaxies & Cosmology (HEAC II) 5 points, ht-2006 Teacher: Göran Östlin Lecture 8 Contents: - Active Galactic Nuclei - Galaxy formation theory.

Galaxy Formation Theory

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Page 24: Galaxies & Cosmology (HEAC II) · Galaxies & Cosmology (HEAC II) 5 points, ht-2006 Teacher: Göran Östlin Lecture 8 Contents: - Active Galactic Nuclei - Galaxy formation theory.
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kc = a.k

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Page 30: Galaxies & Cosmology (HEAC II) · Galaxies & Cosmology (HEAC II) 5 points, ht-2006 Teacher: Göran Östlin Lecture 8 Contents: - Active Galactic Nuclei - Galaxy formation theory.

Einstein - de Sitter (Ω = 1, Λ=0)

”Dust”: p=0, so cs = 0

a ∝ t2/3 = 2 / 3t

Ansatz: Δ∝tn Insert into eq. ⇒ n = 2/3 and -1

n=-1 is a decaying mode, the other slowly growing

Δ = ∝ t2/3

Page 31: Galaxies & Cosmology (HEAC II) · Galaxies & Cosmology (HEAC II) 5 points, ht-2006 Teacher: Göran Östlin Lecture 8 Contents: - Active Galactic Nuclei - Galaxy formation theory.

Open (empty) model (Ω = 0, Λ=0)

a ∝ t

Δ∝tn ⇒ n = 0 and -1No growing mode

If Ω < 1, and Ω ≠ 0, then Ω rapidply approaches unity for small scale factors, so Δ can grow until z ≈ 1/Ω0 - 1

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Page 53: Galaxies & Cosmology (HEAC II) · Galaxies & Cosmology (HEAC II) 5 points, ht-2006 Teacher: Göran Östlin Lecture 8 Contents: - Active Galactic Nuclei - Galaxy formation theory.
Page 54: Galaxies & Cosmology (HEAC II) · Galaxies & Cosmology (HEAC II) 5 points, ht-2006 Teacher: Göran Östlin Lecture 8 Contents: - Active Galactic Nuclei - Galaxy formation theory.
Page 55: Galaxies & Cosmology (HEAC II) · Galaxies & Cosmology (HEAC II) 5 points, ht-2006 Teacher: Göran Östlin Lecture 8 Contents: - Active Galactic Nuclei - Galaxy formation theory.
Page 56: Galaxies & Cosmology (HEAC II) · Galaxies & Cosmology (HEAC II) 5 points, ht-2006 Teacher: Göran Östlin Lecture 8 Contents: - Active Galactic Nuclei - Galaxy formation theory.
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Page 59: Galaxies & Cosmology (HEAC II) · Galaxies & Cosmology (HEAC II) 5 points, ht-2006 Teacher: Göran Östlin Lecture 8 Contents: - Active Galactic Nuclei - Galaxy formation theory.

Measuring Clustering- Count in cells- 2-point corellation function

Page 60: Galaxies & Cosmology (HEAC II) · Galaxies & Cosmology (HEAC II) 5 points, ht-2006 Teacher: Göran Östlin Lecture 8 Contents: - Active Galactic Nuclei - Galaxy formation theory.

Cosmic shear

Challenging!- Effect oneach individualgalaxy tiny- Only visiblethrough laregand deepsamples