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CHANDRA AND VERY LARGE ARRAY OBSERVATIONS OF THE NEARBY Sd GALAXY NGC 45

  • Authors: Thomas G. Pannuti, Douglas A. Swartz, Seppo Laine, Eric M. Schlegel, Christina K. Lacey, William P. Moffitt, Biswas Sharma, Aaron M. Lackey-Stewart, Alekzander R. Kosakowski, Miroslav D. Filipović, and Jeffrey L. Payne

2015 The Astronomical Journal 150 91.

  • Provider: AAS Journals

Caption: Figure 6.

Chandra image of the background galaxy cluster CXOU J001354.2-231254.7 with contours showing IRAC emission overlaid depicting emission detected by IRAC at Channel 1 (3.6 μm). The contours are placed at the levels of 0.22 and 0.57 MJy/sr and the color scale is in counts s−1 pixel−1, where one square pixel corresponds to 0.″5 × 0.″5. See Section 6.

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