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Autor:
Ritacco, A., Pérez, J. F. Macías, Ponthieu, N., Adam, R., Ade, P., André, P., Aumont, J., Beelen, A., Benoît, A., Bideaud, A., Billot, N., Bourrion, O., Bracco, A., Calvo, M., Catalano, A., Coiffard, G., Comis, B., D'Addabbo, A., De Petris, M., Désert, F. X., Doyle, S., Goupy, J., Kramer, C., Lagache, G., Leclercq, S., Lestrade, J. F., Mauskopf, P., Mayet, F., Maury, A., Monfardini, A., Pajot, F., Pascale, E., Perotto, L., Pisano, G., Iglesias, M. Rebolo, Revéret, V., Rodriguez, L., Romero, C., Roussel, H., Ruppin, F., Schuster, K., Sievers, A., Siringo, G., Thum, C., Triqueneaux, S., Tucker, C., Wiesemeyer, H., Zylka, R.
Publikováno v:
A&A 664, C1 (2022)
The Crab nebula is a supernova remnant exhibiting a highly polarized synchrotron radiation at radio and millimeter wavelengths. It is the brightest source in the microwave sky with an extension of 7 by 5 arcminutes and commonly used as a standard can
Externí odkaz:
http://arxiv.org/abs/1804.09581
