output
19952026
most citedPlanck 2015 results. XIII. Cosmological parameters

10.6k citations

Showing 2024 · astro-ph.SRShow all

22 papers · 2 filters

astro-ph.SR2024★ 5 cited

Multiwavelength high-resolution polarimetric imaging of second-generation disc around post-AGB binary IRAS 08544-4431 with SPHERE

Kateryna Andrych, Devika Kamath, Hans Van Winckel +4

Exploring the formation and evolution of second-generation circumbinary discs around evolved binary stars, such as post-Asymptotic Giant Branch (post-AGB) and post-Red Giant Branch…

astro-ph.SR2024★ 6 cited

Multiplicity of Galactic Cepheids from long-baseline interferometry V. High-accuracy orbital parallax and mass of SU Cygni

A. Gallenne, N. R. Evans, P. Kervella +23

Cepheid masses are particularly necessary to help solving the mass discrepancy, while independent distance determinations provide crucial test of the period-luminosity relation and…

astro-ph.SR2024★ 9 cited

A tell-tale tracer for externally irradiated protoplanetary disks: comparing the [CI] 8727 A line and ALMA observations in proplyds

Mari-Liis Aru, Karina Mauco, Carlo F. Manara +15

The evolution of protoplanetary disks in regions with massive OB stars is influenced by externally driven winds that deplete the outer parts of disks. These winds have previously b…

astro-ph.SR2024★ 3 cited

HD 34736: An intensely magnetised double-lined spectroscopic binary with rapidly-rotating chemically peculiar B-type components

E. Semenko, O. Kochukhov, Z. Mikulášek +21

We report the results of a comprehensive study of the spectroscopic binary (SB2) system HD 34736 hosting two chemically peculiar (CP) late B-type stars. Using new and archival obse…

astro-ph.SR2024★ 6 cited

The grazing angle icy protoplanetary disk PDS 453

Laurine Martinien, François Ménard, Gaspard Duchêne +12

PDS 453 is a rare highly inclined disk where the stellar photosphere is seen at grazing incidence on the disk surface. Our goal is take advantage of this geometry to constrain the…

astro-ph.SR2024★ 14 cited

Investigating 39 Galactic Wolf-Rayet stars with VLTI/GRAVITY: Uncovering A Long Period Binary Desert

K. Deshmukh, H. Sana, A. Mérand +16

Wolf-Rayet stars (WRs) are one of the final evolutionary stages of massive stars and immediate progenitors of stellar-mass black holes. Their multiplicity forms an important anchor…

astro-ph.SR2024★ 29 cited

The cool brown dwarf Gliese 229 B is a close binary

Jerry W. Xuan, A. Mérand, W. Thompson +76

Owing to their similarities with giant exoplanets, brown dwarf companions of stars provide insights into the fundamental processes of planet formation and evolution. From their orb…

astro-ph.SR2024★ 6 cited

Multiband polarimetric imaging of HD 34700 with SCExAO/CHARIS

Minghan Chen, Kellon Lawson, Timothy D. Brandt +5

We present Subaru/SCExAO + CHARIS broadband (JHK) integral field spectroscopy of HD 34700 A in polarized light. CHARIS has the unique ability to obtain polarized integral field ima…

astro-ph.SR2024★ 15 cited

Chemical tracers of a highly eccentric AGB-main sequence star binary

T. Danilovich, J. Malfait, M. Van de Sande +32

Binary interactions have been proposed to explain a variety of circumstellar structures seen around evolved stars, including asymptotic giant branch (AGB) stars and planetary nebul…

astro-ph.SR2024★ 8 cited

A kinematical study of the launching region of the blueshifted HH 46/47 outflow with SINFONI K-band observations

M. Birney, C. Dougados, E. T. Whelan +3

Studying outflows is important as they may significantly contribute to angular momentum removal from the star/disk system, affecting disk evolution and planet formation. To investi…

astro-ph.SR2024★ 4 cited

Jet formation in post-AGB binaries: Confronting cold magnetohydrodynamic disc wind wind models with observations

Toon De Prins, Hans Van Winckel, Jonathan Ferreira +4

Aims: We consider cold self-similar magnetohydrodynamic (MHD) disc wind solutions to describe jets that are launched from the circumcompanion accretion discs in post-AGB binaries.…

astro-ph.SR2024★ 9 cited

A new dimension in the variability of AGB stars: convection patterns size changes with pulsation

A. Rosales-Guzmán, J. Sanchez-Bermudez, C. Paladini +16

Stellar convection plays an important role in atmospheric dynamics, wind formation and the mass-loss processes in Asymptotic Giant Branch (AGB) stars. However, a direct characteriz…

astro-ph.SR2024★ 4 cited

Astrometric and photometric characterization of Tel B combining two decades of observations

P. H. Nogueira, C. Lazzoni, A. Zurlo +11

Tel is an 18 Myr system with a 2.09 M A-type star and an M7-M8 brown dwarf companion, Tel B, separated by 4.2'' (208 au). High-contrast imaging campaigns over 20…

astro-ph.SR2024★ 8 cited

FAUST XV. A disk wind mapped by CHOH and SiO in the inner 300 au of the NGC 1333 IRAS 4A2 protostar

M. De Simone, L. Podio, L. Chahine +23

Context. Understanding the connection between outflows, winds, accretion and disks in the inner protostellar regions is crucial for comprehending star and planet formation process.…

astro-ph.SR2024★ 36 cited

A magnetic massive star has experienced a stellar merger

A. J. Frost, H. Sana, L. Mahy +13

Massive stars (those larger than 8 solar masses at formation) have radiative envelopes that cannot sustain a dynamo, the mechanism that produces magnetic fields in lower-mass stars…

astro-ph.SR2024★ 27 cited

Kaleidoscope of irradiated disks: MUSE observations of proplyds in the Orion Nebula Cluster. I. Sample presentation and ionization front sizes

Mari-Liis Aru, Karina Mauco, Carlo F. Manara +10

In the Orion Nebula Cluster (ONC), protoplanetary disks exhibit ionized gas clouds in the form of a striking teardrop shape as massive stars irradiate the disk material. We present…

astro-ph.SR2024★ 31 cited

JWST study of the DG Tau B disk wind candidate: I -- Overview and Nested H/CO outflows

Valentin Delabrosse, Catherine Dougados, Sylvie Cabrit +5

The origin and impact of outflows on proto-planetary disks and planet formation are key open questions. DG Tau B, a Class I protostar with a structured disk and a striking rotating…

astro-ph.SR2024

ALMA Observations of Molecular Line Emission from High-excitation Bipolar Planetary Nebulae

Paula Moraga Baez, Joel H. Kastner, Jesse Bublitz +7

We present early results from our program of ALMA Band 6 (1.3mm) molecular line mapping of a sample of nearby, well-studied examples of high-excitation, bipolar/pinched-waist and m…

astro-ph.SR2024★ 10 cited

Long period modulation of the classical T Tauri star CI Tau: evidence for an eccentric close-in massive planet at 0.17 au

R. Manick, A. P. Sousa, J. Bouvier +13

Detecting planets within protoplanetary disks around young stars is essential for understanding planet formation and evolution. However, planet detection using the radial velocity…

astro-ph.SR2024★ 8 cited

Magnetically driven winds from accretion disks in post-asymptotic giant branch binaries

Olivier Verhamme, Jacques Kluska, Jonathan Ferreira +4

Context. Jets are commonly detected in post-asymptotic giant branch (post-AGB) binaries and originate from an accretion process onto the companion of the post-AGB primary. These je…

astro-ph.SR2024

Cataclysmic Variables and the disc instability model in the Gaia DR3 colour-magnitude diagram

Guillaume Dubus, Carine Babusiaux

Cataclysmic Variables (CVs) are semi-detached binaries composed of a white dwarf orbiting a lower-mass K or M star. We investigate whether CVs are responsible for a new intriguing…

astro-ph.SR2024★ 10 cited

Mid-infrared evidence for iron-rich dust in the multi-ringed inner disk of HD 144432

J. Varga, L. B. F. M. Waters, M. Hogerheijde +40

Context. Rocky planets form by the concentration of solid particles in the inner few au regions of planet-forming disks. Their chemical composition reflects the materials in the di…