A Survey of Velocity Features in Perseus - PowerPoint PPT Presentation

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A Survey of Velocity Features in Perseus

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Title: A Survey of Velocity Features in Perseus


1
A Survey of Velocity Features in
Perseus
  • Michelle BorkinSenior Thesis PresentationMay
    12, 2006

2
A Survey of Velocity Features
in Perseus
3
Star (and Planet) Formation As We Understand It
Disk Jet
Star-Forming Globule
4
Whats an HH knot?
5
Giant Outflows
Greyscale shows ambient 1000 ptcl/cc gas
Red shows 100 ptcl/cc gas moving away from us
Blue shows 100 ptcl/cc gas moving toward us
H. Arces Thesis 2001
6
VLSR 3.4 km/s
3.4 km/s
7
VLSR 3.6 km/s
8
VLSR 3.8 km/s
9
VLSR 4.0 km/s
10
VLSR 4.2 km/s
11
VLSR 4.4 km/s
12
VLSR 4.6 km/s
13
VLSR 4.8 km/s
14
VLSR 5.0 km/s
15
VLSR 5.2 km/s
16
VLSR 5.4 km/s
17
VLSR 5.6 km/s
18
VLSR 5.8 km/s
19
VLSR 6.0 km/s
20
VLSR 6.2 km/s
21
VLSR 6.4 km/s
22
VLSR 6.6 km/s
23
VLSR 6.8 km/s
24
VLSR 7.0 km/s
25
VLSR 7.2 km/s
26
VLSR 7.4 km/s
27
VLSR 7.6 km/s
28
VLSR 7.8 km/s
29
VLSR 8.0 km/s
30
VLSR 8.2 km/s
31
VLSR 8.4 km/s
32
VLSR 8.6 km/s
33
VLSR 8.8 km/s
8.8 km/s
34
Barnards Perseus
35
Giant Outflows
Greyscale shows ambient 1000 ptcl/cc gas
Red shows 100 ptcl/cc gas moving away from us
Blue shows 100 ptcl/cc gas moving toward us
H. Arces Thesis 2001
36
Spectral Line Outflow Mapping
Usually
In Extreme Cases
37
Outflows
Note not drawn to scale.
Based on H. Arce Thesis 2001.
38
3D Slicer
39
3D Slicer
40
A Survey of Velocity Features
in Perseus
41
Outflow Identification
IRAS Sources
Red Shifted points
HH Objects
Known Outflow Sources
SCF points
Blue Shifted points
42
Outflow Identification
Red Shifted points
HH Objects
Known Outflow Sources
c2d Sources
IRAS Sources
SCF points
Blue Shifted points
43
B5
44
B5
45
B5 Results
Region 1 (B5)
46
B5 Results
Summation of all the spectra in Region 1
Gaussian fit
All outflows
previously detected outflows
47
Results and Conclusions
  • 216 high velocity points were identified across
    Perseus
  • In the three regions cataloged, 20 new outflows
    were found
  • 1 new shell was found spanning Regions 5 and 6
    (across L1448 and NGC 1333)
  • Known outflows do not account for all of the
    observed high velocity gas.

48
Future Research
IRAS Sources
Red Shifted points
HH Objects
Known Outflow Sources
SCF points
Blue Shifted points
49
Questions?
For more information, go to http//www.cfa.harva
rd.edu/COMPLETE/ http//www.cfa.harvard.edu/COMPL
ETE/astromed/ http//iic.harvard.edu
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