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1by Tubiana, C., Snodgrass, C., Bertini, I., Mottola, S., Vincent, J.-B., Lara López, Luisa M., Fornasier, S., Knollenberg, J., Thomas, N., Fulle, M., Agarwal, J., Bodewits, D., Ferri, F., Güttler, C., Gutierrez, P. J., La Forgia, F, Lowry, S., Magrin, S., Oklay, N., Pajola, M., Rodrigo, R., Sierks, H., A’Hearn, M. F., Angrilli, F., Barbieri, C., Barucci, M. A., Bertaux, J.-L., Cremonese, G., Da Deppo, V., Davidsson, B., De Cecco, M., Debei, S., Groussin, O., Hviid, S., Ip, W-H., Jorda, L., Keller, H. U., Koschny, D., Kramm, R., Kührt, E., Küppers, M., Lazzarin, M., Lamy, P., Lopez Moreno, J., Marzari, F., Michalik, H., Naletto, G., Rickman, H., Sabau, L., Wenzel, K. P.“... photometry, we investigated how the comet brightness varies with heliocentric distance. 67P was likely...”
Published in Astronomy & Astrophysics (2015)
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