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Autor:
Kobulnicky, Henry A., Kiminki, Daniel C., Lundquist, Michael J., Burke, Jamison, Chapman, James, Keller, Erica, Lester, Kathryn, Rolen, Emily K., Topel, Eric, Bhattacharjee, Anirban, Smullen, Rachel A., Alvarez, Carlos A. Vargas, Runnoe, Jessie C., Dale, Daniel A., Brotherton, Michael M.
We analyze orbital solutions for 48 massive multiple-star systems in the Cygnus OB2 Association, 23 of which are newly presented here, to find that the observed distribution of orbital periods is approximately uniform in log P for P<45 d, but it is n
Externí odkaz:
http://arxiv.org/abs/1406.6655