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Autor:
Erik Dennihy, Amy Bonsor, Anna F. Pala, Jay Farihi, Laura K. Rogers, Thomas G. Wilson, Andrew Swan, Kate Y. L. Su, Scott J. Kenyon, Siyi Xu, Paul W. Cauley, Seth Redfield, T. von Hippel, R van Lieshout, William T. Reach, Odette Toloza, John H. Debes, Boris T. Gänsicke
The infrared dust emission from the white dwarf GD 56 is found to rise and fall by 20% peak-to-peak over 11.2 yr, and is consistent with ongoing dust production and depletion. It is hypothesized that the dust is produced via collisions associated wit
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a3aa401ee53f242533bd2c289f55d561
http://wrap.warwick.ac.uk/108985/1/WRAP-dust-production-depletion-evolved-planetary-systems-Gaensicke-2018.pdf
http://wrap.warwick.ac.uk/108985/1/WRAP-dust-production-depletion-evolved-planetary-systems-Gaensicke-2018.pdf