Characterization of the long-period companions of the exoplanet host stars: HD 196885, HD 1237 and HD 27442. VLT/NACO and SINFONI near-infrared, follow-up imaging and spectroscopy

Details Characterization of the long-period companions of the exoplanet host stars: HD 196885, HD 1237 and HD 27442. VLT/NACO and SINFONI near-infrared, follow-up imaging and spectroscopy Characterization of the long-period companions of the exoplanet host stars: HD 196885, HD 1237 and HD 27442. VLT/NACO and SINFONI near-infrared, follow-up imaging and spectroscopy

Nov 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007a%26a...475..723c&link_type=abstract

Astronomy and Astrophysics, Volume 475, Issue 2, November IV 2007, pp.723-727

Astronomy and Astrophysics

Astrophysics

14

Instrumentation: High Angular Resolution, Stars: Binaries: Close, Stars: Low-Mass, Brown Dwarfs, Stars: Planetary Systems

Scientific paper

Aims:We present the results of near-infrared, follow-up imaging and spectroscopic observations at VLT, aimed at characterizing the long-period companions of the exoplanet host stars HD 196885, HD 1237 and HD 27442. The three companions were previously discovered in the course of our CFHT and VLT coronographic imaging survey dedicated to the search for faint companions of exoplanet host stars. Methods: We used the NACO near-infrared adaptive optics instrument to obtain astrometric follow-up observations of HD 196885 A and B. The long-slit spectroscopic mode of NACO and the integral field spectrograph SINFONI were used to carry out a low-resolution spectral characterization of the three companions HD 196885 B, HD 1237 B and HD 27442 B between 1.4 and 2.5 μm. Results: We can now confirm that the companion HD 196885 B is comoving with its primary exoplanet host star, as previously shown for HD 1237 B and HD 27442 B. We find that both companions HD 196885 B and HD 1237 B are low-mass stars of spectral type M1±1V and M4±1V respectively. HD 196885 AB is one of the closer (~23 AU) resolved binaries known to host an exoplanet. This system is then ideal for carrying out a combined radial velocity and astrometric investigation of the possible impact of the binary companion on the planetary system formation and evolution. Finally, we confirm via spectroscopy that HD 27442 B is a white dwarf companion, the third one to be discovered orbiting an exoplanet host star, following HD 147513 and Gliese 86. The detection of the broad Brγ line of hydrogen indicates a white dwarf atmosphere dominated by hydrogen.
Based on ESO observing programs 075.C-0825(A), 275.B-5057A and 077.C-0444(A).

Affiliated with

Also associated with

No associations

Rating

Characterization of the long-period companions of the exoplanet host stars: HD 196885, HD 1237 and HD 27442. VLT/NACO and SINFONI near-infrared, follow-up imaging and spectroscopy does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Characterization of the long-period companions of the exoplanet host stars: HD 196885, HD 1237 and HD 27442. VLT/NACO and SINFONI near-infrared, follow-up imaging and spectroscopy, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Characterization of the long-period companions of the exoplanet host stars: HD 196885, HD 1237 and HD 27442. VLT/NACO and SINFONI near-infrared, follow-up imaging and spectroscopy will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1695822