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Related papers: HD 106906 b: A planetary-mass companion outside a …

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Context. Though only a handful of extrasolar planets have been discovered via direct imaging, each of these discoveries had tremendous impact on our understanding of planetary formation, stellar formation and cool atmosphere physics. Aims.…

Solar and Stellar Astrophysics · Physics 2016-10-05 P. Delorme , J. Gagné , J. H. Girard , A. M. Lagrange , G. Chauvin , M-E. Naud , D. Lafrenière , R. Doyon , A. Riedel , M. Bonnefoy , L. Malo

Chauvin et al. 2005 imaged a co-moving companion at ~260 AU from the young star AB Pic A. Evolutionary models predictions based on J H K photometry of AB Pic b suggested a mass of ~13 - 14 MJup, placing the object at the deuterium-burning…

Earth and Planetary Astrophysics · Physics 2015-05-14 M. Bonnefoy , G. Chauvin , P. Rojo , F. Allard , A. -M. Lagrange , D. Homeier , C. Dumas , J. -L. Beuzit

We present Herschel spatially resolved images of the debris disc orbiting the subgiant Kappa CrB. Not only are these the first resolved images of a debris disc orbiting a subgiant, but Kappa CrB is a rare example of an intermediate mass…

Earth and Planetary Astrophysics · Physics 2015-06-15 Amy Bonsor , Grant M. Kennedy , Justin R. Crepp , John A. Johnson , Mark C. Wyatt , Bruce Sibthorpe , Kate Y. L. Su

With the uniquely high contrast within 0.1" (\Delta mag(L') = 5-6.5 magnitudes) available using Sparse Aperture Masking (SAM) with NACO at VLT, we detected asymmetry in the flux from the Herbig Fe star HD 142527 with a barycenter emission…

HD 95086 is an intermediate-mass debris-disk-bearing star. VLT/NaCo $3.8 \mu m$ observations revealed it hosts a $5\pm2 \mathrm{M}_{Jup}$ companion (HD 95086 b) at $\simeq 56$ AU. Follow-up observations at 1.66 and 2.18 $\mu m$ yielded a…

Young circumstellar disks are of prime interest to understand the physical and chemical conditions under which planet formation takes place. Only very few detections of planet candidates within these disks exist, and most of them are…

Earth and Planetary Astrophysics · Physics 2018-09-12 M. Keppler , M. Benisty , A. Müller , Th. Henning , R. van Boekel , F. Cantalloube , C. Ginski , R. G. van Holstein , A. -L. Maire , A. Pohl , M. Samland , H. Avenhaus , J. -L. Baudino , A. Boccaletti , J. de Boer , M. Bonnefoy , G. Chauvin , S. Desidera , M. Langlois , C. Lazzoni , G. Marleau , C. Mordasini , N. Pawellek , T. Stolker , A. Vigan , A. Zurlo , T. Birnstiel , W. Brandner , M. Feldt , M. Flock , J. Girard , R. Gratton , J. Hagelberg , A. Isella , M. Janson , A. Juhasz , J. Kemmer , Q. Kral , A. -M. Lagrange , R. Launhardt , A. Matter , F. Ménard , J. Milli , P. Mollière , J. Olofsson , L. Perez , P. Pinilla , C. Pinte , S. P. Quanz , T. Schmidt , S. Udry , Z. Wahhaj , J. P. Williams , E. Buenzli , M. Cudel , C. Dominik , R. Galicher , M. Kasper , J. Lannier , D. Mesa , D. Mouillet , S. Peretti , C. Perrot , G. Salter , E. Sissa , F. Wildi , L. Abe , J. Antichi , J. -C. Augereau , A. Baruffolo , P. Baudoz , A. Bazzon , J. -L. Beuzit , P. Blanchard , S. S. Brems , T. Buey , V. De Caprio , M. Carbillet , M. Carle , E. Cascone , A. Cheetham , R. Claudi , A. Costille , A. Delboulbé , K. Dohlen , D. Fantinel , P. Feautrier , T. Fusco , E. Giro , D. Gisler , L. Gluck , C. Gry , N. Hubin , E. Hugot , M. Jaquet , D. Le Mignant , M. Llored , F. Madec , Y. Magnard , P. Martinez , D. Maurel , M. Meyer , O. Moeller-Nilsson , T. Moulin , L. Mugnier , A. Origne , A. Pavlov , D. Perret , C. Petit , J. Pragt , P. Puget , P. Rabou , J. Ramos , F. Rigal , S. Rochat , R. Roelfsema , G. Rousset , A. Roux , B. Salasnich , J. -F. Sauvage , A. Sevin , C. Soenke , E. Stadler , M. Suarez , M. Turatto , L. Weber

Binary stars and higher-order multiple systems are an ubiquitous outcome of star formation, especially as the system mass increases. The companion mass-ratio distribution is a unique probe into the conditions of the collapsing cloud core…

Solar and Stellar Astrophysics · Physics 2016-08-03 Kevin Gullikson , Adam Kraus , Sarah Dodson-Robinson

We report the detection of a low-mass companion orbiting the solar-type star HD178911B, the distant component of the stellar triple system HD178911. The variability of HD178911B was first detected using radial-velocity measurements obtained…

To understand the influence of additional wide stellar companions on planet formation, it is necessary to determine the fraction of multiple stellar systems amongst the known extrasolar planet population. We target recently discovered…

Earth and Planetary Astrophysics · Physics 2015-06-04 C. Ginski , M. Mugrauer , M. Seeliger , T. Eisenbeiss

In this paper we present the results of the SPHERE observation of the HD 284149 system, aimed at a more detailed characterisation of both the primary and its brown dwarf companion. We observed HD 284149 in the near-infrared with SPHERE,…

We report on the discovery of the companion star to the millisecond pulsar PSR J1835-3259B in the Galactic globular cluster NGC 6652. Taking advantage of deep photometric archival observations acquired through the Hubble Space Telescope in…

High Energy Astrophysical Phenomena · Physics 2023-05-17 J. Chen , M. Cadelano , C. Pallanca , F. Ferraro , B. Lanzoni , A. Istrate , M. Burgay , P. Freire , T. Gautam , A. Possenti , A. Ridolfi

We present results from an adaptive optics survey for substellar and stellar companions to Sun-like stars. The survey targeted 266 F5-K5 stars in the 3Myr to 3Gyr age range with distances of 10-190pc. Results from the survey include the…

Astrophysics · Physics 2009-11-13 Stanimir Metchev , Lynne Hillenbrand

We present the first multi-wavelength (near-infrared; $1.1 - 2.4$ $\mu m$) imaging of HD 36546's debris disk, using the Subaru Coronagraphic Extreme Adaptive Optics (SCExAO) system coupled with the Coronagraphic High Angular Resolution…

We used the Magellan adaptive optics (MagAO) system and its VisAO CCD camera to image the young low mass brown dwarf companion CT Chamaeleontis B for the first time at visible wavelengths. We detect it at r', i', z', and Ys. With our new…

Debris disks are usually detected through the infrared excess over the photospheric level of their host star. The most favorable stars for disk detection are those with spectral types between A and K, while the statistics for debris disks…

We explore the probable chemical signature of planet formation in the remarkable binary system HD 106515. The A star hosts a massive long-period planet with 9 MJup detected by radial velocity. We also refine stellar and planetary parameters…

Solar and Stellar Astrophysics · Physics 2019-05-08 C. Saffe , E. Jofre , P. Miquelarena , M. Jaque Arancibia , M. Flores , F. M. Lopez , A. Collado

We report precise Doppler measurements of HD 142022 obtained during the past six years with the CORALIE echelle spectrograph at La Silla Observatory together with a few additional observations made recently with the HARPS echelle…

Astrophysics · Physics 2009-11-11 A. Eggenberger , M. Mayor , D. Naef , F. Pepe , D. Queloz , N. C. Santos , S. Udry , C. Lovis

We present infrared H- and K-band spectra of a companion candidate 3" north of the young star GSC 08047-00232, a probable member of the nearby young Horologium association. From previously obtained JHK-band colors and the magnitude…

Astrophysics · Physics 2009-11-10 Ralph Neuhaeuser , Eike Guenther

We obtained deep H- and K-band images of DENIS-P J104814-395606 using SofI and the speckle camera SHARP-I at the ESO-3.5m-NTT as well as QUIRC at the Mauna Kea 2.2m telescope between December 2000 and June 2001. The target was recently…