✦ LIBER ✦

The Ogle-Tr-56 Star–Planet System

✍ Scribed by Todd Vaccaro; Walter Van Hamme

Book ID: 106352612
Publisher: Springer Netherlands
Year: 2005
Tongue: English
Weight: 135 KB
Volume: 296
Category: Article
ISSN: 0004-640X
DOI: 10.1007/s10509-005-4453-8

No coin nor oath required. For personal study only.

📜 SIMILAR VOLUMES

New constraints from the Hα line for the

New constraints from the Hα line for the temperature of the transiting planet host star OGLE-TR-10

✍ M. Ammler-von Eiff; N.C. Santos 📂 Article 📅 2008 🏛 John Wiley and Sons 🌐 English ⚖ 582 KB

Planets and Planet-Sized Binaries from t

Planets and Planet-Sized Binaries from the OGLE Transit Survey

✍ Frédéric Pont; François Bouchy 📂 Article 📅 2006 🏛 Springer Netherlands 🌐 English ⚖ 221 KB

The abundance of Galactic planets from O

The abundance of Galactic planets from OGLE-III 2002 microlensing data

✍ Colin Snodgrass; Keith Horne; Yiannis Tsapras 📂 Article 📅 2004 🏛 John Wiley and Sons 🌐 English ⚖ 350 KB

Astrophysics: Evolution of star–planet s

Astrophysics: Evolution of star–planet systems

✍ Bath, Geoffrey 📂 Article 📅 1984 🏛 Nature Publishing Group 🌐 English ⚖ 273 KB

K-band transit and secondary eclipse pho

K-band transit and secondary eclipse photometry of exoplanet OGLE-TR-113b

✍ I. A. G. Snellen; E. Covino 📂 Article 📅 2007 🏛 John Wiley and Sons 🌐 English ⚖ 750 KB

Habitable Planet Formation in Binary Sta

Habitable Planet Formation in Binary Star Systems

✍ Daniel P Whitmire; John J Matese; Lee Criswell; Seppo Mikkola 📂 Article 📅 1998 🏛 Elsevier Science 🌐 English ⚖ 287 KB

## AU), or when the secondary has a very low mass and near The accretion of planetesimals from a turbulent gas and circular orbit as in the Sun-Jupiter system. The discrepancy dust nebula is not well understood theoretically even in with the present numerical study is due in part to the different