output
19952026
most citedPlanck 2015 results. XIII. Cosmological parameters

10.6k citations

Showing 2023 · astro-ph.SRShow all

42 papers · 2 filters

astro-ph.SR2023

NIKA2 observations of dust grain evolution from star-forming filament to T-Tauri disk: Preliminary results from NIKA2 observations of the Taurus B211/B213 filament

Q. Nguyen-Luong, R. Adam, P. Ade +51

To understand the evolution of dust properties in molecular clouds in the course of the star formation process, we constrain the changes in the dust emissivity index from star-form…

astro-ph.SR2023★ 7 cited

Correlations between laboratory line lists for FeH, CrH, and NiH and M-star spectra collected with ESPaDOnS and SPIRou

P. Crozet, J. Morin, A. J. Ross +9

Molecular bands of metal oxides and hydrides dominate the optical and near-infrared spectra of M dwarfs. High-resolution spectra of these bands have immense potential for determini…

astro-ph.SR2023★ 28 cited

Monitoring the young planet host V1298 Tau with SPIRou: planetary system and evolving large-scale magnetic field

B. Finociety, J. -F. Donati, P. I. Cristofari +15

We report results of a spectropolarimetric monitoring of the young Sun-like star V1298~Tau based on data collected with the near-infrared spectropolarimeter SPIRou at the Canada-Fr…

astro-ph.SR2023★ 15 cited

VLTI/GRAVITY Observations and Characterization of the Brown Dwarf Companion HD 72946 B

W. O. Balmer, L. Pueyo, T. Stolker +96

Tension remains between the observed and modeled properties of substellar objects, but objects in binary orbits, with known dynamical masses can provide a way forward. HD 72946 B i…

astro-ph.SR2023★ 13 cited

Multiples among B stars in the Scorpius-Centaurus association

R. Gratton, V. Squicciarini, V. Nascimbeni +13

We discuss the properties of companions to B stars in the Scorpius-Centaurus association (age ~15 Myr, 181 B-stars). We gathered available data combining high contrast imaging samp…

astro-ph.SR2023★ 6 cited

Star-disk interactions in the strongly accreting T Tauri Star S CrA N

H. Nowacki, E. Alecian, K. Perraut +11

Aims : We aimed at constraining the accretion-ejection phenomena around the strongly-accreting Northern component of the S CrA young binary system (S CrA N) by deriving its magneti…

astro-ph.SR2023★ 8 cited

Binaries masses and luminosities with Gaia DR3

S. Chevalier, C. Babusiaux, T. Merle +1

The recent Gaia third data release (DR3) has brought some new exciting data about stellar binaries. It provides new opportunities to fully characterize more stellar systems and con…

astro-ph.SR2023

Magnetic fields & rotation periods of M dwarfs from SPIRou spectra

J. -F. Donati, L. T. Lehmann, P. I. Cristofari +17

We present near-infrared spectropolarimetric observations of a sample of 43 weakly- to moderately-active M dwarfs, carried with SPIRou at the Canada-France-Hawaii Telescope in the…

astro-ph.SR2023★ 15 cited

The Great Dimming of the hypergiant star RW Cephei: CHARA Array images and spectral analysis

N. Anugu, F. Baron, D. R. Gies +15

The cool hypergiant star RW Cephei is currently in a deep photometric minimum that began several years ago. This event bears a strong similarity to the Great Dimming of the red sup…

astro-ph.SR2023★ 35 cited

Monitoring the large-scale magnetic field of AD~Leo with SPIRou, ESPaDOnS and Narval. Toward a magnetic polarity reversal?

S. Bellotti, J. Morin, L. T. Lehmann +23

One manifestation of dynamo action on the Sun is the 22-yr magnetic cycle, exhibiting a polarity reversal and a periodic conversion between poloidal and toroidal fields. For M dwar…

astro-ph.SR2023★ 7 cited

Predicting convective blueshift and radial-velocity dispersion due to granulation for FGK stars

S. Dalal, R. D. Haywood, A. Mortier +2

To detect Earth-mass planets using the Doppler method, a major obstacle is to differentiate the planetary signal from intrinsic stellar variability (e.g., pulsations, granulation,…

astro-ph.SR2023★ 8 cited

Reconstructing the mid-infrared environment in the stellar merger remnant V838 Monocerotis

Muhammad Zain Mobeen, Tomasz Kamiński, Alexis Matter +15

V838 Mon is a stellar merger remnant that erupted in 2002 in a luminous red novae event. Although it is well studied in the optical, near infrared and submillimeter regimes, its st…

astro-ph.SR2023★ 8 cited

Resolving the Binary Components of the Outbursting Protostar HBC 494 with ALMA

Pedro Henrique Nogueira, Alice Zurlo, Sebastián Pérez +15

Episodic accretion is a low-mass pre-main sequence phenomenon characterized by sudden outbursts of enhanced accretion. These objects are classified into two: protostars with elevat…

astro-ph.SR2023★ 7 cited

Imaging the warped dusty disk wind environment of SU Aurigae with MIRC-X

Aaron Labdon, Stefan Kraus, Claire L. Davies +12

SU Aurigae is a widely studied T Tauri star and here we present original state-of-the-art interferometric observations with better uv and baseline coverage than previous studies. W…

astro-ph.SR2023★ 9 cited

Discovery of Magnetospheric Interactions in the Doubly-Magnetic Hot Binary Lupi

Ayan Biswas, Barnali Das, Poonam Chandra +6

Magnetic fields are extremely rare in close, hot binaries, with only 1.5\% of such systems known to contain a magnetic star. The eccentric Lupi system stands out in this popula…

astro-ph.SR2023★ 19 cited

The GRAVITY young stellar object survey -- XI. Probing the inner disk and magnetospheric accretion region of CI Tau

GRAVITY Collaboration, A. Soulain, K. Perraut +6

Aims: We aim at spatially and spectrally resolving the innermost scale of the young stellar object CI Tau to constrain the inner disk properties and better understand the magnetosp…

astro-ph.SR2023★ 22 cited

The surprising evolution of the shadow on the TW Hya disk

J. Debes, R. Nealon, R. Alexander +8

We report new total intensity visible light high contrast imaging of the TW Hya disk taken with the Space Telescope Imaging Spectrograph (STIS) on the Hubble Space Telescope (HST).…

astro-ph.SR2023★ 12 cited

Transition disc nature of post-AGB binary systems confirmed by mid-infrared interferometry

A. Corporaal, J. Kluska, H. Van Winckel +4

Many properties of circumbinary discs around evolved post-asymptotic giant branch (post-AGB) binary systems are similar to those of protoplanetary discs around young stars. The def…

astro-ph.SR2023★ 10 cited

FU Orionis disk outburst: evidence for a gravitational instability scenario triggered in a magnetically dead zone

G. Bourdarot, J-P. Berger, G. Lesur +10

Context: FUors outbursts are a crucial stage of accretion in young stars. However a complete mechanism at the origin of the outburst still remains missing. Aims: We aim at constrai…

astro-ph.SR2023★ 79 cited

The magnetic field and multiple planets of the young dwarf AU~Mic

J. -F. Donati, P. I. Cristofari, B. Finociety +25

In this paper we present an analysis of near-infrared spectropolarimetric and velocimetric data of the young M dwarf AU Mic, collected with SPIRou at the Canada-France-Hawaii teles…

astro-ph.SR2023★ 25 cited

FAUST VIII. The protostellar disk of VLA 1623-2417 W and its streamers imaged by ALMA

S. Mercimek, L. Podio, C. Codella +25

More than 50% of solar-mass stars form in multiple systems. It is therefore crucial to investigate how multiplicity affects the star and planet formation processes at the protostel…

astro-ph.SR2023★ 40 cited

Constraining atmospheric parameters and surface magnetic fields with : an application to SPIRou spectra

P. I. Cristofari, J. -F. Donati, C. P. Folsom +8

We report first results on a method aimed at simultaneously characterising atmospheric parameters and magnetic properties of M dwarfs from high-resolution nIR spectra recorded with…

astro-ph.SR2023★ 35 cited

Characterisation of stellar activity of M dwarfs. I. Long-timescale variability in a large sample and detection of new cycles

L. Mignon, N. Meunier, X. Delfosse +7

M dwarfs are active stars that exhibit variability in chromospheric emission and photometry at short and long timescales, including long cycles that are related to dynamo processes…

astro-ph.SR2023★ 14 cited

FAUST VII. Detection of A Hot Corino in the Prototypical Warm Carbon-Chain Chemistry Source IRAS 15398-3359

Yuki Okoda, Yoko Oya, Logan Francis +16

We have observed the low-mass protostellar source, IRAS 153983359, at a resolution of 0.2-0.3, as part of the Atacama Large Millimeter/Submillimeter Array Large Program…