On the Fundamental Mass-Period Functions of Extrasolar Planets - INSPIRE

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On the Fundamental Mass-Period Functions of Extrasolar Planets

Dec, 2009

15 pages

Published in:

Astrophys.J.Suppl. 186 (2010) 48-62

e-Print:

0912.2585 [astro-ph.EP]

DOI:

10.1088/0067-0049/186/1/48

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Abstract: (arXiv)

Employing a catalog of 175 extrasolar planets (exoplanets) detected by the Doppler-shift method, we constructed the independent and coupled mass-period functions. It is the first time in this field that the selection effect is considered in the coupled mass-period functions. Our results are consistent with those in Tabachnik and Tremaine (2002) with the major differences that we obtain a flatter mass function but a steeper period function. Moreover, our coupled mass-period functions show that about 2.5 percent of stars would have a planet with mass between Earth Mass and Neptune Mass, and about 3 percent of stars would have a planet with mass between Neptune Mass and Jupiter Mass.

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