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ALMAGAL IV. Morphological comparison of molecular and thermal dust emission using the histogram of oriented gradients (HOG) method

Fuente: arXiv
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Bibliographic Details
Main Authors: Mininni, C., Molinari, S., Soler, J. D., Sánchez-Monge, Á., Coletta, A., Benedettini, M., Traficante, A., Schisano, E., Elia, D., Pezzuto, S., Nucara, A., Schilke, P., Battersby, C., Ho, P. T. P., Béltran, M. T., Beuther, H., Fuller, G. A., Jones, B., Klessen, R. S., Zhang, Q., Walch, S., Tang, Y., Ahmadi, A., Allande, J., Avison, A., Brogan, C. L., De Angelis, F., Fontani, F., Hennebelle, P., Hunter, T. R., Johnston, K. G., Koch, P., Kuiper, R., Law, C. Y., Lis, D. C., Liu, S., Liu, T., Moscadelli, L., Möller, T., Rigby, A. J., Rygl, K. L. J., Sanhueza, P., Testi, L., Su, Y. N., van der Tak, F. F. S., Wells, M. R. A., Bronfman, L., Zhang, T., Zinnecker, H.
Format: Preprint
Published: 2025
Subjects:
Astrophysics of Galaxies
Online Access:
Acceder al recurso
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