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First Results from a 1.3 cm Expanded Very Large Array Survey of Massive Protostellar Objects: G35.03+0.35

  • Authors: C. L. Brogan, T. R. Hunter, C. J. Cyganowski, R. K. Friesen, C. J. Chandler, and R. Indebetouw

Brogan et al. 2011 The Astrophysical Journal Letters 739 L16.

  • Provider: AAS Journals

Caption: Figure 2.

Zoomed-in view of the NE and SW cores showing the NH 3 (1,1) integrated intensity in color scale with VLA 3.6 cm continuum contours (0.1, 0.3, 2, and 7 mJy beam −1) from Cyganowski et al. (2011) superposed in blue; the three brightest centimeter continuum sources are labeled CM1, CM2, and CM3. (a) SMA 1.3 mm continuum is shown in white contours (levels: 7, 30, and 90 mJy beam −1) and the synthesized beams of the EVLA (yellow), VLA (blue), and SMA (white) are shown in the lower left corner. (b) White contours show the integrated intensity of NH 3 (2,2) (levels: 25, 50, 75, and 117 mJy beam −1 km s −1). (c) Contours show the integrated intensity of NH 3 (3,3) (white; 30, 60, and 120 mJy beam −1 km s −1) and (6,6) (cyan; 13, 17, and 22 mJy beam −1 km s −1). In all panels, the locations of two new 25 GHz CH 3OH masers are cyan triangles, and 6.7 and 44 GHz CH 3OH masers from Figure 1 are also shown.

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