Obliquities of hot Jupiter host stars: Evidence for tidal interactions and primordial misalignments

MLA

Massachusetts Institute of Technology. Department of Physics, et al. “Obliquities of Hot Jupiter Host Stars: Evidence for Tidal Interactions and Primordial Misalignments.” ArXiv, 2013. EBSCOhost, widgets.ebscohost.com/prod/customlink/proxify/proxify.php?count=1&encode=0&proxy=&find_1=&replace_1=&target=https://search.ebscohost.com/login.aspx?direct=true&site=eds-live&scope=site&db=edsoai&AN=edsoai.ocn828156823&authtype=sso&custid=ns315887.

APA

Massachusetts Institute of Technology. Department of Physics, MIT Kavli Institute for Astrophysics and Space Research, Albrecht, S. H., Winn, J. N., Johnson, J. A., Howard, A. W., Marcy, G. W., Butler, R. P., Arriagada, P., Crane, J. D., Shectman, S. A., Thompson, I. B., Hirano, T., Bakos, G. A., & Hartman, J. D. (2013). Obliquities of hot Jupiter host stars: Evidence for tidal interactions and primordial misalignments. ArXiv.

Chicago

Massachusetts Institute of Technology. Department of Physics, MIT Kavli Institute for Astrophysics and Space Research, Simon H. Albrecht, Joshua Nathan Winn, John Asher Johnson, Andrew W. Howard, Geoffrey W. Marcy, et al. 2013. “Obliquities of Hot Jupiter Host Stars: Evidence for Tidal Interactions and Primordial Misalignments.” ArXiv. http://widgets.ebscohost.com/prod/customlink/proxify/proxify.php?count=1&encode=0&proxy=&find_1=&replace_1=&target=https://search.ebscohost.com/login.aspx?direct=true&site=eds-live&scope=site&db=edsoai&AN=edsoai.ocn828156823&authtype=sso&custid=ns315887.