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ALMA Observations of Supernova Remnant N49 in the Large Magellanic Cloud. II. Non-LTE Analysis of Shock-heated Molecular Clouds

  • Authors: H. Sano, Y. Yamane, J. Th. van Loon, K. Furuya, Y. Fukui, R. Z. E. Alsaberi, A. Bamba, R. Enokiya, M. D. Filipović, R. Indebetouw, T. Inoue, A. Kawamura, M. Lakićević, C. J. Law, N. Mizuno, T. Murase, T. Onishi, S. Park, P. P. Plucinsky, J. Rho, A. M. S. Richards, G. Rowell, M. Sasaki, J. Seok, P. Sharda, L. Staveley-Smith, H. Suzuki, T. Temim, K. Tokuda, K. Tsuge, K. Tachihara

H. Sano et al 2023 The Astrophysical Journal 958 .

  • Provider: AAS Journals

Caption: Figure 5.

Time evolution of kinematic temperature T kin at the cloud center after the supernova event that generates SNR N49. Colors indicate the assumed cosmic-ray ionization rate ζ from 3 × 10−17 s−1 to 1 × 10−14 s−1. The star symbol indicates the observed values of T kin for the ambient or pre-shocked clouds at the age of N49 (4800 yr).

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