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The Circumnuclear Starburst Ring In NGC 1097 Beverly Thackeray-Lacko CSUSB.

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Presentation on theme: "The Circumnuclear Starburst Ring In NGC 1097 Beverly Thackeray-Lacko CSUSB."— Presentation transcript:

1 The Circumnuclear Starburst Ring In NGC 1097 http://apod.nasa.gov/apod/image/1501/NGC1097_newmaster3starshadows.jpg Beverly Thackeray-Lacko CSUSB

2 Nearby Well Studied Interesting Features Orientation Lots of data across many frequencies What we know.... 14.5 MPC 45 Million Ly Barred Spiral Galaxy AGN Starbursting Nuclear Ring 700 Parsecs in Radius 5 M ʘ per year 140 Million M ʘ Low Luminosity 5,500 Light-years in Radius Face-On

3 Starbursting circum-nuclear ring https://www.eso.org/public/images/eso0534a/

4 What is an SED?: Dale et al. 2007 http://almaost.jb.man.ac.uk/ http://candels-collaboration.blogspot.com/2012/08/the-multi- wavelength-shapes-of-galaxies.html https://www.eso.org/public/images/eso0534a/

5 What does SED tell us? Age of stellar population Star formation rate Dust qualities AGN properties http://ned.ipac.caltech.edu/level5/March13/Lagache/Figures/figure1.jpghttp://ned.ipac.caltech.edu/level5/March05/Leitherer/Figures/figure6.jpg

6 Ultraviolet Optical Radio Infrared DATA GALEX Poor resolution Bands 1 and 2 Band 7: Cycle 0 3.2 mm Wavelength 2.2 arcsec = 155 Pc 349 GHz 8.55 mm Wavelength 93 GHz IRAC CTIO 1.5m telescope B,V,R,I 1.52 arcsec = 107 Pc ~ 4 arcsec ~ 2 arcsec ~ 2.4 arcsec 2.2 X 1.64 arcsec 1.52 X 1.21 arcsec Band 3: ALMA http://irsa.ipac.caltech.edu/data/SPITZER/S4G/galaxies/NGC1097.html http://irsa.ipac.caltech.edu/data/SPITZER/SINGS/ http://galex.stsci.edu/GR6/

7 Reduce DATA Regrid Convert Units Convolve How to create an SED: Cycle 0 ALMA Define ring? Jy / beam Use worst resolution Re-pixels images Outline Ring Subtract background 1.5 x radius of outer ring IRAC band 1 3.6 μm IRAC band 2 4.5 μm Galex FUV 1350-1780 Å Galex NUV 1770-2730 Å CTIO I.90 μm CTIO R.70 μm CTIO V.54 μm CTIO B.43 μm ALMA 7.85 mm. Alma 3 contours at 4 σ

8 Results:

9 SED’s are challenging! There is more work ahead Conclusions and Future work: Examine regions of interest within ring Fit an SED to circumnuclear ring Create error bars

10 Diversity

11 Acknowledgements: Sabrina Stierwalt Loreto Barcos Drew Brisbin Kertik Sheth Arielle Moullet NRAO National Astronomy Consortium https://science.nrao.edu/opportunities/student-programs/nac/ Kimberly Sokal Data Analysts Brittney High Adam Trapp


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