Figure 4 from ALMA CO Observations of Gamma-Ray Supernova Remnant N132D in the Large Magellanic Cloud: Possible Evidence for Shocked Molecular Clouds Illuminated by Cosmic-Ray Protons

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

ALMA CO Observations of Gamma-Ray Supernova Remnant N132D in the Large Magellanic Cloud: Possible Evidence for Shocked Molecular Clouds Illuminated by Cosmic-Ray Protons

Authors: H. Sano, P. P. Plucinsky, A. Bamba, P. Sharda, M. D. Filipović, C. J. Law, R. Z. E. Alsaberi, Y. Yamane, K. Tokuda, F. Acero, M. Sasaki, J. Vink, T. Inoue, S. Inutsuka, J. Shimoda, K. Tsuge, K. Fujii, F. Voisin, N. Maxted, G. Rowell, T. Onishi, A. Kawamura, N. Mizuno, H. Yamamoto, K. Tachihara, and Y. Fukui

2020 The Astrophysical Journal 902 53.

Provider: AAS Journals

Caption: Figure 4.

Averaged line profiles of ¹²CO(J = 3–2) (red) and H I (blue and cyan) toward the SNR N132D. The blue and cyan spectra were extracted from regions inside and outside a circle with radius ﹩30^{\prime\prime} ﹩ at the center position of (﹩{\alpha }_{{\rm{J}}2000}﹩, ﹩{\delta }_{{\rm{J}}2000}﹩) ∼ (﹩{05}^{{\rm{h}}}{25}^{{\rm{m}}}02\buildrel{\rm{s}}\over{.} 88﹩, ﹩-69^\circ 38^{\prime} 34\buildrel{\prime\prime}\over{.} 8﹩). The red spectrum was produced by averaging the whole spectra shown in Figure 2(b).

Other Images in This Article

Copyright and Terms & Conditions