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The Magellanic System: A History of Discovery

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The MS in History (very abridged) Henrietta Leavitt and the SMC Cepheids ... And dust: 1% of ISM mass 0.1mm. heating/cooling. catalyst for molecule formation ... – PowerPoint PPT presentation

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Title: The Magellanic System: A History of Discovery


1
The Magellanic System A History of Discovery
  • Annie Hughes, Swinburne University of Technology

2
Resumen
  • Overview of The Magellanic System
  • The MS in History (very abridged)
  • Henrietta Leavitt and the SMC Cepheids
  • WIMPs vs MACHOs
  • Supernova 1987A
  • Extended Stellar Populations in the MCs?
  • Formation of the Magellanic Stream?

3
Sky View
4
Sky View
The Local Group
5
Sky View
6
(No Transcript)
7
But galaxies are more than stars
  • A galaxy is made of
  • dark matter (gt90 of galaxy mass)
  • stars
  • interstellar medium (ISM, lt1 of mass)

8
But galaxies are more than stars
  • The ISM consists of gas
  • mostly hydrogen, some helium and traces of
    heavier elements, which astronomers call metals

H2, cold
H, cool/warm
H, warm/hot
9
Sky View
10
Sky View
11
Sky View
12
Sky View
13
Sky View
14
Sky View
15
Emu in the Sky
16
Aboriginal Astronomy
17
Al Sufi and The White Ox
18
Cape Clouds
19
John Herschel
20
John Herschel
21
Henrietta Leavitt
  • Employed as computer at Harvard College
    Observatory in 1893 to catalogue the brighness of
    stars from Arequipa plates.

22
Finding Cepheids in the SMC
23
The Period-Luminosity Relation
24
Hubble Discovers the Universe
25
M100 Cepheids
26
Zwicky Discovers Dark Matter
27
Dark Matter Candidates
  • MACHOs
  • Massive Compact Halo Objects
  • brown dwarfs, planets, black holes
  • astronomers

28
Gravitational Lensing
29
MACHO Microlensing
30
The MACHO Project
  • Question What fraction of Milky Ways halo
    consists of MACHOs?
  • Experiment Six years of photometric monitoring
    of 12 million stars in the LMC and 5 million
    stars in the SMC.

31
MACHO Microlensing
  • MACHO candidate
  • LMC GPE 1
  • (051444.5 -684800)

32
Conclusions from MACHO
  • Detected 13 to 17 events in LMC
  • 9 x 1010 M? of MACHOs within 50 kpc of MW
  • MACHOs are objects with mass 0.5 M?
  • 20 of MWs halo is MACHOs
  • MACHOs cannot be all the missing mass

33
Flashback to 1987
34
Flashback to 1987
35
What is a supernova?
36
Stellar Evolution
37
Stellar Evolution
38
Flashback to 1987
39
Confirmation!
40
Formation of the Stream
  • Tidal interaction?
  • Ram pressure stripping?
  • Blow out from 30 Doradus?

41
An extended stellar population
  • RGB stars from LMC observed up to 23º from LMC
    optical centre
  • What??!

Majewski et al 2009
42
A conclusion (sort of)
  • We still have a lot to learn about the Magellanic
    System!

43
(No Transcript)
44
Cepheid Variables
45
Pulsation
  • Pulsation mechanism is the Eddington valve
  • He is more opaque than He
  • Radiation pushes outwards gravity pulls inwards

He
He
He
Dim
Bright
Dim
46
Sky View
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