ELODIE metallicity-biased search for transiting Hot Jupiters III. A hot Jupiter orbiting the star HD 185269

C. Moutou; B. Loeillet; F. Bouchy; R. Da Silva; M. Mayor; F. Pont; D. Queloz; N. C. Santos; D. Ségransan; S. Udry; S. Zucker

doi:10.1051/0004-6361:20066029

ELODIE metallicity-biased search for transiting Hot Jupiters III. A hot Jupiter orbiting the star HD 185269

C. Moutou, B. Loeillet, F. Bouchy, R. Da Silva, M. Mayor, F. Pont, D. Queloz, N. C. Santos, D. Ségransan, S. Udry, S. Zucker

Research output: Contribution to journal › Article › peer-review

Abstract

We present new results of a search for extrasolar planets. The survey uses radial-velocity techniques and focuses on metal-rich stars. We used radial velocity measurements obtained with the echelle spectrograph ELODIE at the Observatoire de Haute Provence. New data have revealed a planetary companion to the slightly evolved star HD 185269. It belongs to the hot Jupiter class of planets, with a projected mass M sin i = 1.0 M_Jup and period P = 6.84 days. We describe the measurements that led to this discovery and discuss the orbital solution.

Original language	English
Pages (from-to)	327-329
Number of pages	3
Journal	Astronomy and Astrophysics
Volume	458
Issue number	1
DOIs	https://doi.org/10.1051/0004-6361:20066029
State	Published - Oct 2006
Externally published	Yes

Keywords

Planetary systems
Stars: individual: HD 185269
Techniques: radial velocities

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10.1051/0004-6361:20066029

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title = "ELODIE metallicity-biased search for transiting Hot Jupiters III. A hot Jupiter orbiting the star HD 185269",

abstract = "We present new results of a search for extrasolar planets. The survey uses radial-velocity techniques and focuses on metal-rich stars. We used radial velocity measurements obtained with the echelle spectrograph ELODIE at the Observatoire de Haute Provence. New data have revealed a planetary companion to the slightly evolved star HD 185269. It belongs to the hot Jupiter class of planets, with a projected mass M sin i = 1.0 MJup and period P = 6.84 days. We describe the measurements that led to this discovery and discuss the orbital solution.",

keywords = "Planetary systems, Stars: individual: HD 185269, Techniques: radial velocities",

author = "C. Moutou and B. Loeillet and F. Bouchy and {Da Silva}, R. and M. Mayor and F. Pont and D. Queloz and Santos, {N. C.} and D. S{\'e}gransan and S. Udry and S. Zucker",

year = "2006",

month = oct,

doi = "10.1051/0004-6361:20066029",

language = "אנגלית",

volume = "458",

pages = "327--329",

journal = "Astronomy and Astrophysics",

issn = "0004-6361",

publisher = "EDP Sciences",

number = "1",

}

ELODIE metallicity-biased search for transiting Hot Jupiters III. A hot Jupiter orbiting the star HD 185269. / Moutou, C.; Loeillet, B.; Bouchy, F.; Da Silva, R.; Mayor, M.; Pont, F.; Queloz, D.; Santos, N. C.; Ségransan, D.; Udry, S.; Zucker, S.

In: Astronomy and Astrophysics, Vol. 458, No. 1, 10.2006, p. 327-329.

Research output: Contribution to journal › Article › peer-review

TY - JOUR

T1 - ELODIE metallicity-biased search for transiting Hot Jupiters III. A hot Jupiter orbiting the star HD 185269

AU - Moutou, C.

AU - Loeillet, B.

AU - Bouchy, F.

AU - Da Silva, R.

AU - Mayor, M.

AU - Pont, F.

AU - Queloz, D.

AU - Santos, N. C.

AU - Ségransan, D.

AU - Udry, S.

AU - Zucker, S.

PY - 2006/10

Y1 - 2006/10

N2 - We present new results of a search for extrasolar planets. The survey uses radial-velocity techniques and focuses on metal-rich stars. We used radial velocity measurements obtained with the echelle spectrograph ELODIE at the Observatoire de Haute Provence. New data have revealed a planetary companion to the slightly evolved star HD 185269. It belongs to the hot Jupiter class of planets, with a projected mass M sin i = 1.0 MJup and period P = 6.84 days. We describe the measurements that led to this discovery and discuss the orbital solution.

AB - We present new results of a search for extrasolar planets. The survey uses radial-velocity techniques and focuses on metal-rich stars. We used radial velocity measurements obtained with the echelle spectrograph ELODIE at the Observatoire de Haute Provence. New data have revealed a planetary companion to the slightly evolved star HD 185269. It belongs to the hot Jupiter class of planets, with a projected mass M sin i = 1.0 MJup and period P = 6.84 days. We describe the measurements that led to this discovery and discuss the orbital solution.

KW - Planetary systems

KW - Stars: individual: HD 185269

KW - Techniques: radial velocities

UR - http://www.scopus.com/inward/record.url?scp=33750261999&partnerID=8YFLogxK

U2 - 10.1051/0004-6361:20066029

DO - 10.1051/0004-6361:20066029

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AN - SCOPUS:33750261999

VL - 458

SP - 327

EP - 329

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

SN - 0004-6361

IS - 1

ER -

ELODIE metallicity-biased search for transiting Hot Jupiters III. A hot Jupiter orbiting the star HD 185269

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Keywords

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