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PROTOPLANETARY DISKS IN THE HOSTILE ENVIRONMENT OF CARINA

  • Authors: A. Mesa-Delgado, L. Zapata, W. J. Henney, T. H. Puzia, and Y. G. Tsamis

2016 The Astrophysical Journal Letters 825 L16.

  • Provider: AAS Journals

Caption: Figure 2.

Top: RGB images of the EGGs 104–593 (left-hand side) and 105–600 (right-hand side) constructed from narrow-band Hubble Space Telescope images from Wide Field Camera 3 (WFC3), Advanced Camera for Surveys (ACS), and Wide Field/Planetary Camera 2 (WFPC2). For 104–593, WFC3 visual band filters in lines of [O III] (blue), [N II] (green), and [S II] (red). For 105–600, ACS visual band [N II] filter (blue), WFPC2 visual band [S II] filter (green), and WFC3 infrared [Fe II] filter (red). The images also show the Herbig-Haro objects HH1066 in 104–593 and HH1006 in 105–600. Bottom: ALMA detections at 1.3 mm continuum emission. The white contours represent values at ﹩3.8\sigma ﹩, ﹩5.3\sigma ﹩, ﹩6.8\sigma ﹩, ﹩8.3\sigma ﹩, and ﹩9.8\sigma ﹩ mJy beam−1 for 104–593, and ﹩2.9\sigma ﹩, ﹩3.4\sigma ﹩, ﹩3.9\sigma ﹩, ﹩4.4\sigma ﹩, ﹩5.0\sigma ﹩, and ﹩5.5\sigma ﹩ mJy beam−1 for 105–600. The white ellipses show the beam size of ﹩0\buildrel{\prime\prime}\over{.} 03\times 0\buildrel{\prime\prime}\over{.} 02﹩.

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