output
19932026
Showing 2018 · astro-ph.EPShow all

70 papers · 2 filters

astro-ph.EP2018★ 22 cited

Detection and characterization of an ultra-dense sub-Neptune planet orbiting the Sun-like star HD 119130

R. Luque, G. Nowak, E. Pallé +51

We present the discovery and characterization of a new transiting planet from Campaign 17 of the Kepler extended mission K2. HD 119130 b is a warm sub-Neptune on a 17-d orbit aroun…

astro-ph.EP2018

The effect of carbon grain destruction on the chemical structure of protoplanetary disks

Chen-En Wei, Hideko Nomura, Jeong-Eun Lee +3

The bulk composition of the Earth is dramatically carbon poor compared to that of the interstellar medium, and this phenomenon extends to the asteroid belt. To interpret this carbo…

astro-ph.EP2018★ 46 cited

Gas density perturbations induced by forming planet(s) in the AS 209 protoplanetary disk as seen with ALMA

Cécile Favre, Davide Fedele, Luke Maud +6

The formation of planets occurs within protoplanetary disks surrounding young stars, resulting in perturbation of the gas and dust surface densities. Here, we report the first evid…

astro-ph.EP2018★ 275 cited

Ground-based detection of an extended helium atmosphere in the Saturn-mass exoplanet WASP-69b

Lisa Nortmann, Enric Pallé, Michael Salz +25

Hot gas giant exoplanets can lose part of their atmosphere due to strong stellar irradiation, affecting their physical and chemical evolution. Studies of atmospheric escape from ex…

astro-ph.EP2018★ 158 cited

Detection of He I Å absorption on HD 189733 b with CARMENES high-resolution transmission spectroscopy

M. Salz, S. Czesla, P. C. Schneider +35

We present three transit observations of HD 189733 b obtained with the high-resolution spectrograph CARMENES at Calar Alto. A strong absorption signal is detected in the near-infra…

astro-ph.EP2018★ 243 cited

Spectrally resolved helium absorption from the extended atmosphere of a warm Neptune-mass exoplanet

R. Allart, V. Bourrier, C. Lovis +7

Stellar heating causes atmospheres of close-in exoplanets to expand and escape. These extended atmospheres are difficult to observe because their main spectral signature - neutral…

astro-ph.EP2018★ 83 cited

A search for accreting young companions embedded in circumstellar disks: High-contrast H imaging with VLT/SPHERE

G. Cugno, S. P. Quanz, S. Hunziker +37

Aims: We want to detect and quantify observables related to accretion processes occurring locally in circumstellar disks, which could be attributed to young forming planets. We foc…

astro-ph.EP2018★ 44 cited

HD219666b: A hot-Neptune from TESS Sector 1

M. Esposito, D. J. Armstrong, D. Gandolfi +73

We report on the confirmation and mass determination of a transiting planet orbiting the old and inactive G7 dwarf star HD219666 (Mstar = 0.92 +/- 0.03 MSun, Rstar = 1.03 +/- 0.03…

astro-ph.EP2018★ 23 cited

The Little Dippers: Transits of Star-grazing Exocomets?

Megan Ansdell, Eric Gaidos, Tom L. Jacobs +9

We describe EPIC 205718330 and EPIC 235240266, two systems identified in the K2 data whose light curves contain episodic drops in brightness with shapes and durations similar to th…

astro-ph.EP2018★ 24 cited

Catching a planet: A tidal capture origin for the exomoon candidate Kepler 1625b I

Adrian S. Hamers, Simon F. Portegies Zwart

The (yet-to-be confirmed) discovery of a Neptune-sized moon around the ~3.2 Jupiter-mass planet in Kepler 1625 puts interesting constraints on the formation of the system. In parti…

astro-ph.EP2018★ 81 cited

Multiple water band detections in the CARMENES near-infrared transmission spectrum of HD 189733 b

F. J. Alonso-Floriano, A. Sánchez-López, I. A. G. Snellen +27

Aims: We explore the capabilities of CARMENES for characterizing hot-Jupiter atmospheres by targeting multiple water bands, in particular, those at 1.15 and 1.4 m. Hubble Space…

astro-ph.EP2018★ 73 cited

Variable Outer Disk Shadowing Around the Dipper Star RX J1604.3-2130

P. Pinilla, M. Benisty, J. de Boer +6

Low brightness dips have been recently observed in images of protoplanetary disks, and they are believed to be shadows by the inner disk. We present VLT/SPHERE polarimetric differe…

astro-ph.EP2018★ 72 cited

The Ring Structure in the MWC 480 Disk Revealed by ALMA

Yao Liu, Giovanni Dipierro, Enrico Ragusa +20

Gap-like structures in protoplanetary disks are likely related to planet formation processes. In this paper, we present and analyze high resolution (0.17*0.11 arcsec) 1.3 mm ALMA c…

astro-ph.EP2018★ 35 cited

WASP-166b: a bloated super-Neptune transiting a V = 9 star

Coel Hellier, D. R. Anderson, A. H. M. J. Triaud +21

We report the discovery of WASP-166b, a super-Neptune planet with a mass of 0.1 Mjup (1.9 Mnep) and a bloated radius of 0.63 Rjup. It transits a V = 9.36, F9V star in a 5.44-d orbi…

astro-ph.EP2018★ 69 cited

PynPoint: a modular pipeline architecture for processing and analysis of high-contrast imaging data

Tomas Stolker, Markus J. Bonse, Sascha P. Quanz +4

The direct detection and characterization of planetary and substellar companions at small angular separations is a rapidly advancing field. Dedicated high-contrast imaging instrume…

astro-ph.EP2018★ 42 cited

The Formation of Solar System Analogs in Young Star Clusters

Simon Portegies Zwart

The Solar system was once rich in the short-lived radionuclide (SLR) Al\, but deprived in Fe. Several models have been proposed to explain these anomalous abundances…

astro-ph.EP2018★ 21 cited

Observability of molecular species in a nitrogen dominated atmosphere for 55 Cancri e

Yamila Miguel

One of the key goals of exoplanet science is the atmospheric characterisation of super-Earths. Atmospheric abundances provide insight on the formation and evolution of those planet…

astro-ph.EP2018★ 14 cited

Constraining the period of the ringed secondary companion to the young star J1407 with photographic plates

R. T. Mentel, M. A. Kenworthy, D. A. Cameron +13

Context. The 16 Myr old star 1SWASP J140747.93-394542.6 (V1400 Cen) underwent a series of complex eclipses in May 2007, interpreted as the transit of a giant Hill sphere filling de…

astro-ph.EP2018★ 25 cited

K2-140b and K2-180b - Characterization of a hot Jupiter and a mini-Neptune from the K2 mission

J. Korth, Sz. Csizmadia, D. Gandolfi +40

We report the independent discovery and characterization of two K2 planets: K2-180b, a mini-Neptune-size planet in an 8.9-day orbit transiting a V = 12.6 mag, metal-poor ([Fe/H] =$…

astro-ph.EP2018★ 9 cited

Data calibration for the MASCARA and bRing instruments

G. J. J. Talens, E. R. Deul, R. Stuik +8

Aims: MASCARA and bRing are photometric surveys designed to detect variability caused by exoplanets in stars with . Such variability signals are typically small and requ…

astro-ph.EP2018★ 19 cited

Magnetically induced termination of giant planet formation

A. J. Cridland

Here a physical model for terminating giant planet formation is outlined and compared to other methods of late-stage giant planet formation. As has been pointed out before, gas acc…

astro-ph.EP2018★ 114 cited

Evidence for a massive dust-trapping vortex connected to spirals: a multi-wavelength analysis of the HD~135344B protoplanetary disk

P. Cazzoletti, E. F. van Dishoeck, P. Pinilla +6

Spiral arms, rings and large scale asymmetries are structures observed in high resolution observations of protoplanetary disks, and it appears that some of the disks showing spiral…

astro-ph.EP2018★ 141 cited

Dynamical Constraints on the HR 8799 Planets with GPI

Jason J. Wang, James R. Graham, Rebekah Dawson +52

The HR 8799 system uniquely harbors four young super-Jupiters whose orbits can provide insights into the system's dynamical history and constrain the masses of the planets themselv…

astro-ph.EP2018★ 32 cited

On water delivery in the inner solar nebula: Monte Carlo simulations of forsterite hydration

Martina D'Angelo, Stephanie Cazaux, Inga Kamp +2

Endogenous or exogenous, dry or wet, various scenarios have been so far depicted for the origin of water on our Solar Systems rocky bodies. Hydrated silicates found in meteorites a…