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The Greatest Explosions since the Big Bang:

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Mosaic II = 36'x36' ESO WFI = 34'x33' OmegaCam = 1ox1o. 75' Student seminar ... Only if observing close to the ecliptic. Generally not associated with a galaxy ... – PowerPoint PPT presentation

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Title: The Greatest Explosions since the Big Bang:


1
The Greatest Explosions since the Big Bang
Supernovae!
2
Up for discussion
  • Why are they so important?
  • How do we find them?
  • How do we classify them?
  • What is it that explodes?
  • Major discoveries using supernovae

3
The importance of Supernovae
  • Nucleosynthesis of chemical elements
  • Star formation histories
  • Chemical evolution
  • Distance measurement
  • Peculiar velocity studies
  • Cosmological models
  • The nature of Gamma Ray Bursts

4
Can you spot the new SN?
Photographic Plates UKS 6.6ox6.6o Wide
Field Imagers MaCHO 45x45 Mosaic II
36x36 ESO WFI 34x33 OmegaCam 1ox1o
5
Searching for Supernovae
Construct a Template
6
Searching for Supernovae - 2
New Image with SN
Shifted to Template
7
Searching for Supernovae - 3
Adjusted for Seeing and transparency
Subtracted
8
Searching for Supernovae - 4
Red Image
Blue Image
Red Subtraction
Blue Subtraction
Red Template
Blue Template
9
Searching for Supernovae - 5
  • Cosmic Ray
  • Rare to have coincident CRs in 2 images
  • Asteroid
  • Only if observing close to the ecliptic
  • Generally not associated with a galaxy in the
    template
  • Variable Star
  • Associated with a star in the template
  • Recurrent over many observations
  • AGN
  • Located in the centre of the galaxy

10
How many supernovae do we find?
11
And the winner is --- KAIT!
  • 76cm telescope _at_ Lick
  • Robotic telescope to search for SNe and monitor
    other events (e.g. GRBs/Novae)

12
Classification
Type Ic
t 1 week
13
SN Progenitors
14
Type II, Type Ib, Type Ic Progenitors
15
Type Ia Progenitors
16
Its all good!
17
Or is it?
(Type Ia)
18
Type IIn
vs
Type II
19
Type Ia
Type IIn
20
SN 1997cy
21
SN 1999E
22
Confused?
Type Ic
Type Ia
Type II
Type IIn
core-collapse
Type Ib
23
Supernova classification tree
24
Nucleosynthesis
Type Ia (white dwarf binary)
Core-collapse (massive stars)
Ni, Co, Mn, Fe gt Fe
C, O, N gtFe
25
Late-time spectra of SNe
26
Light Curves of Supernovae
27
Light Curves of Type Ia SNe
28
Brighter SlowerFainter Faster
29
Luminosity-Decline Rate Relation
30
Template Fitting MCLS ?m15
31
Template Fitting - Stretch
32
Template Fitting - how good is it?
  • But why does this work at all

33
Measuring Distances with SNIa
  • Have absolute magnitude of the SN through
    template fitting methods
  • Have apparent brightness of the SN through
    photometry

DISTANCES accurate to 7
34
What have we learned from Type Ia Supernovae?
35
The Universe is Accelerating!
  • SNe at high-Z are fainter than expected
  • Acceleration started sometime in the last 10
    billion years

36
The Universe is Accelerating!
  • Best cosmological model
  • ?M 0.28
  • ?? 0.72

37
What Does this Mean?
  • The Mundane Astronomers have been fooled by
    supernovae into believing the Universe is
    accelerating. Perhaps supernovae were
    intrinsically fainter in the past and therefore
    look further away?

38
Probably not )
  • CMB data alone suggests a flat universe with ?gt0
  • Any 2 of CMB/SN/LSS taken together indicate an
    accelerating Universe with a dark energy
    component of 70

39
What Does this Mean?
  • The Heretical General Relativity (though sacred
    in Physics) may be wrong. Since the observations
    are interpreted through the predictions of
    General Relativity, the conclusion that the
    Universe is accelerating may also be wrong -/

40
What Does this Mean?
  • The Exciting The Universe is being accelerated
    by some unknown type of energy that is spread
    throughout the cosmos!

41
Where do we go from here?
  • SNAP - SN acceleration probe
  • 2000 SNe/year for 3 years
  • Expansion history to 1

42
What have we learned from core-collapse
Supernovae?
43
Hypernovae long duration GRBs
44
Summary
  • Importance

VERY
  • Nucleosynthesis of chemical elements
  • Measuring Distances/Cosmology
  • Understanding GRBs

45
Summary
  • Discovery

Thank goodness for computers!
  • Initially by eye (I cant bear to think of it!)
  • Now by fully automatic, robotic telescopes

46
Summary
  • Classification Progenitors

Very messy!
  • Basically 2 types
  • Type Ia explosion of a white dwarf binary
  • Core-collapse explosion of a massive star

47
Summary
  • Science

Very EXCITING!
  • Type Ia revealed the accelerating Universe and
    the existence of dark energy
  • Core-collapse are associated with GRBs

48
Who is next to explode?
49
Best Candidate?
  • Bright as a half moon but a point of light, not a
    disk
  • Visible to the naked eye for many months
  • Could be tomorrow, could be in 10,000 years.

Betelgeuse
50
Or perhaps?
51
Interested in Learning More?
http//astronomy.swin.edu.au/lgermany/
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