output
19952026
most citedPlanck 2015 results. XIII. Cosmological parameters

10.6k citations

Showing 2017 · astro-ph.SRShow all

50 papers · 2 filters

astro-ph.SR2017★ 146 cited

The genealogical tree of ethanol: gas-phase formation of glycolaldehyde, acetic acid and formic acid

Dimitrios Skouteris, Nadia Balucani, Cecilia Ceccarelli +5

Despite the harsh conditions of the interstellar medium, chemistry thrives in it, especially in star forming regions where several interstellar complex organic molecules (iCOMs) ha…

astro-ph.SR2017★ 92 cited

The lithium-rotation connection in the 125 Myr-old Pleiades cluster

J. Bouvier, D. Barrado, E. Moraux +9

The evolution of lithium abundance over a star's lifetime is indicative of transport processes operating in the stellar interior. We revisit the relationship between lithium conten…

astro-ph.SR2017★ 82 cited

SPIRou Input Catalogue: Global properties of 440 M dwarfs observed with ESPaDOnS at CFHT

Pascal Fouqué, Claire Moutou, Lison Malo +13

Present and future high-precision radial-velocity spectrometers dedicated to the discovery of low-mass planets orbiting low-mass dwarfs need to focus on the best selected stars to…

astro-ph.SR2017★ 34 cited

HD 156324: a tidally locked magnetic triple spectroscopic binary with a disrupted magnetosphere

M. Shultz, Th. Rivinius, G. A. Wade +3

HD 156324 is an SB3 (B2V/B5V/B5V) system in the Sco OB4 association. The He-strong primary possesses both a strong magnetic field, and H emission believed to originate in its Ce…

astro-ph.SR2017★ 146 cited

The evolution of surface magnetic fields in young solar-type stars II: The early main sequence (250-650 Myr)

C. P. Folsom, J. Bouvier, P. Petit +6

There is a large change in surface rotation rates of sun-like stars on the pre-main sequence and early main sequence. Since these stars have dynamo driven magnetic fields, this imp…

astro-ph.SR2017★ 19 cited

The Scuti pulsations of Pictoris as observed by ASTEP from Antarctica

D. Mékarnia, E. Chapellier, T. Guillot +13

The Antartica Search for Transiting Extrasolar Planets (ASTEP), an automatized 400 mm telescope located at Concordia station in Antarctica, monitored beta Pictoris continuously to…

astro-ph.SR2017★ 32 cited

Magnetic fields of intermediate mass T Tauri stars

A. Lavail, O. Kochukhov, G. A. J. Hussain +3

Aims. In this paper, we aim to measure the strength of the surface magnetic fields for a sample of five intermediate mass T Tauri stars and one low mass T Tauri star from late-F to…

astro-ph.SR2017★ 38 cited

The open flux evolution of a solar-mass star on the main sequence

V. See, M. Jardine, A. A. Vidotto +9

Magnetic activity is known to be correlated to the rotation period for moderately active main sequence solar-like stars. In turn, the stellar rotation period evolves as a result of…

astro-ph.SR2017★ 33 cited

HST Scattered Light Imaging and Modeling of the Edge-on Protoplanetary Disk ESO-H 569

Schuyler G. Wolff, Marshall D. Perrin, Karl Stapelfeldt +6

We present new HST ACS observations and detailed models for a recently discovered edge-on protoplanetary disk around ESO H 569 (a low-mass T Tauri star in the Cha I star forming…

astro-ph.SR2017★ 46 cited

Variability in stellar granulation and convective blueshift with spectral type and magnetic activity. II. From young to old main-sequence K-G-F stars

Nadège Meunier, Lucile Mignon, Anne-Marie Lagrange

The inhibition of small-scale convection in the Sun dominates the long-term radial velocity (RV) variability: it therefore has a critical effect on light exoplanet detectability us…

astro-ph.SR2017★ 155 cited

Seeds Of Life In Space (SOLIS): The organic composition diversity at 300--1000 au scale in Solar-type star forming regions

C. Ceccarelli, P. Caselli, F. Fontani +43

Complex organic molecules have been observed for decades in the interstellar medium. Some of them might be considered as small bricks of the macromolecules at the base of terrestri…

astro-ph.SR2017★ 125 cited

ALMA discovery of a rotating SO/SO flow in HH212. A possible MHD disk wind?

B. Tabone, S. Cabrit, E. Bianchi +7

We wish to constrain the possible contribution of a magnetohydrodynamic disk wind (DW) to the HH212 molecular jet. We mapped the flow base with ALMA Cycle 4 at 0.13" 60 au re…

astro-ph.SR2017★ 206 cited

Direct mapping of the temperature and velocity gradients in discs. Imaging the vertical CO snow line around IM Lupi

C. Pinte, F. Menard, G. Duchene +14

Accurate measurements of the physical structure of protoplanetary discs are critical inputs for planet formation models. These constraints are traditionally established via complex…

astro-ph.SR2017★ 30 cited

Impact of convection and resistivity on angular momentum transport in dwarf novae

N. Scepi, G. Lesur, G. Dubus +1

The eruptive cycles of dwarf novae (DN) are thought to be due to a thermal-viscous instability in the accretion disk surrounding the white dwarf (WD). This model has long been know…

astro-ph.SR2017★ 2 cited

The programme "accurate masses for SB2 components"

Jean-Louis Halbwachs, Frédéric Arenou, Henri M. J. Boffin +11

Accurate stellar masses are requested in order to improve our understanding of stellar interiors, but they are still rather rare. Fortunately, the forthcoming Gaia Mission will pro…

astro-ph.SR2017★ 40 cited

Deuterated methanol on Solar System scale around the HH212 protostar

E. Bianchi, C. Codella, C. Ceccarelli +13

Context: Methanol is thought to be mainly formed during the prestellar phase and its deuterated form keeps memory of the conditions at that epoch. Thanks to the unique combination…

astro-ph.SR2017★ 53 cited

Nitrogen and hydrogen fractionation in high-mass star forming cores from observations of HCN and HNC

L. Colzi, F. Fontani, P. Caselli +3

The ratio between the two stable isotopes of nitrogen, N and N, is well measured in the terrestrial atmosphere (), and in the pre-Solar nebula ().…

astro-ph.SR2017★ 14 cited

A near-infrared interferometric survey of debris-disk stars. VI. Extending the exozodiacal light survey with CHARA/JouFLU

Paul D. Nunez, N. J. Scott, B. Mennesson +11

We report the results of high-angular-resolution observations that search for exozodiacal light in a sample of main sequence stars and sub-giants. Using the "jouvence" of the fiber…

astro-ph.SR2017★ 71 cited

SPIRou Input Catalog: Activity, Rotation and Magnetic Field of Cool Dwarfs

C. Moutou, E. M. Hebrard, J. Morin +7

Based on optical high-resolution spectra obtained with CFHT/ESPaDOnS, we present new measurements of activity and magnetic field proxies of 442 low-mass K5-M7 dwarfs. The objects w…

astro-ph.SR2017★ 4 cited

The wind and the magnetospheric accretion onto the T Tauri star S Coronae Australis at sub-au resolution

R. Garcia Lopez, K. Perraut, A. Caratti o Garatti +70

To investigate the inner regions of protoplanetary disks, we performed near-infrared interferometric observations of the classical TTauri binary system S CrA. We present the first…

astro-ph.SR2017★ 70 cited

In-depth study of moderately young but extremely red, very dusty substellar companion HD206893B

P. Delorme, T. Schmidt, M. Bonnefoy +47

The substellar companion HD206893b has recently been discovered by direct imaging of its disc-bearing host star with the SPHERE instrument. We investigate the atypical properties o…

astro-ph.SR2017★ 15 cited

Magnetic activity and radial velocity filtering of young Suns: The weak-line T Tauri stars Par 1379 and Par 2244

C. A. Hill, A. Carmona, J. -F. Donati +5

We report the results of our spectropolarimetric monitoring of the weak-line T-Tauri stars (wTTSs) Par 1379 and Par 2244, within the MaTYSSE (Magnetic Topologies of Young Stars and…

astro-ph.SR2017★ 88 cited

Consistent dust and gas models for protoplanetary disks: II. Chemical networks and rates

Inga Kamp, Wing-Fai Thi, Peter Woitke +3

Aims. We define a small and large chemical network which can be used for the quantitative simultaneous analysis of molecular emission from the near-IR to the submm. We revise react…

astro-ph.SR2017★ 44 cited

A 80 au cavity in the disk around HD 34282

G. van der Plas, F. Menard, H. Canovas +5

Context: Large cavities in disks are important testing grounds for the mechanisms proposed to drive disk evolution and dispersion, such as dynamical clearing by planets and photo-e…