Bun'ei Sato coauthored the discovery study of the transiting planet HD 149026 b. Combining a transit radius with a radial-velocity mass made its high bulk density informative about planetary interior models. The inference depends on both measured quantities and the assumed composition model.[ref]
The N2K Consortium. II. A Transiting Hot Saturn Around HD 149026 With a Large Dense Core by Bun'ei Sato and others. author list and the described study’s abstract or introductory account
Articles by others on the same topic
There are currently no matching articles.