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AIP Conference Proceedings

Publication date: 2011-03-01
Volume: 1331 Pages: 304 - 309
Publisher: Springer New York LLC

Author:

Jacobs, Valery Ann
Ostensen, Roy ; Van Winckel, Hans ; Bloemen, Steven ; Pápics, Péter ; Raskin, Gert ; Debosscher, Jonas ; Uttenthaler, Stefan ; van Aarle, Els ; Waelkens, Christoffel ; Bauwens, Eva ; Verhoelst, Tijl ; Gielen, Clio ; Lehmann, Holger ; Oreiro Rey, Raquel

Abstract:

A close substellar companion has been claimed to orbit the bright sdB star HD 149382 with a period of 2.391 d. In order to check this important discovery we gathered 26 high resolution spectra over 55 days with the HERMES spectrograph on the 1.2 m Mercator telescope on La Palma, and analyzed the resulting radial velocities. Our data show no sign of any significant radial-velocity periodicities, and from the high precision of our measurements we rule out any RV variations with amplitudes higher than 0.79 km/s on periods shorter than 50 days.