the topology of hi in the smc

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The Topology of HI in the SMC Jeremy Gordon University of Georgia August 2, 2007 Advisors: Dr. Chepurnov Dr. Lazarian

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The Topology of HI in the SMC. Jeremy Gordon University of Georgia August 2, 2007 Advisors: Dr. Chepurnov Dr. Lazarian. Overview:. Small Magellanic Cloud Genus Statistics HI Column Density Map My Project Results. The Small Magellanic Cloud. NGC 292 - PowerPoint PPT Presentation

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Page 1: The Topology of HI in the SMC

The Topology of HI in the SMC

Jeremy GordonUniversity of Georgia

August 2, 2007

Advisors: Dr. Chepurnov Dr. Lazarian

Page 2: The Topology of HI in the SMC

Overview:

Small Magellanic Cloud Genus Statistics HI Column Density Map My Project Results

Page 3: The Topology of HI in the SMC

The Small Magellanic Cloud

NGC 292 RA 00h52m, Dec -72°50’ ~60 kpc distant, covers ~ 4.5° x 4.5° area Knots, filaments, holes, oh my!

Page 4: The Topology of HI in the SMC

Genus Statistics

Initial Developments

2D Genus – ’89

G2 = (isolated high-density regions) – (isolated low-density regions)

Mathematically Speaking:

Page 5: The Topology of HI in the SMC

Genus Statistics, Cont.

Random Distribution:

Genus Shift Δν +Δν ‘swiss-

cheese’ topology -Δν ‘meatball’

topology Kim & Park, 2007

Page 6: The Topology of HI in the SMC

Applications: Turbulence Studies of turbulence utilize the power

spectrum, which contains information on velocity fluctuations

No topological information embedded in the power spectrum, however

Genus analysis is a complementary tool in the study of turbulence

Page 7: The Topology of HI in the SMC

Data and Analysis

Combination of Parkes & ATCAdata

HI: 21 cm line (1420MHz)

Spatial resolution of 29.52”/8.59pc

Effective resolution of ~90”/30pc

Page 8: The Topology of HI in the SMC

HI Column Density Map

Page 9: The Topology of HI in the SMC

Methodology

SMC cropped into 9 overlapping 150x150 regions

‘Entire’ SMC cropped in 400x300 pixel region

Smoothing scale λ ≤ 10% of image length

Page 10: The Topology of HI in the SMC

Results 30-75pc: clump

topology, trending towards neutral shift

Page 11: The Topology of HI in the SMC

Results 30-75pc: clump

topology, trending towards neutral shift

75-125pc: neutral/slight positive shift, hole topology

Page 12: The Topology of HI in the SMC

Results 30-75pc: clump

topology, trending towards neutral shift

75-125pc: neutral/slight positive shift, hole topology

≥ 125pc: shift becoming more negative, clump topology

Page 13: The Topology of HI in the SMC

Results, Cont. 150x150 Regions: Small Scales:

30 pc ≤ λ ≤ 50 pc Medium Scales

50 pc ≤ λ ≤ 75 pc Large Scales

λ ≥ 75 pc Similarities &

Differences

Page 14: The Topology of HI in the SMC

150x150 Results

Page 15: The Topology of HI in the SMC

Conclusion

SMC exhibits a clump topology at small scales

At medium scales, genus shift becomes less negativeneutral/slight positive shift

At large scales, genus shift levels out at a slight negative value

Genus Analysis is an effective, complementary tool in the study of turbulence

Page 16: The Topology of HI in the SMC

References

Gott, J. R., III, Dickinson, M., & Melott, A. L. 1986, ApJ, 306, 341

Kim, S., & Park, C. 2007, ApJ, 663, 244 Melott, A. L., Cohen, A. P., Hamilton, A. J. S., Gott, J. R. I.,

& Weinberg, D. H. 1989, ApJ, 345, 618 Stanimirovic, S., Staveley-Smith, L., Dickey, J. M., Sault,

R. J., & Snowden, S. L. 1999, MNRAS, 302, 417 Staveley-Smith, L., Sault, R. J., Hatzidimitriou, D.,

Kesteven, M. J., & McConnell, D. 1997, MNRAS, 289, 225