Search Publications

Moving structures in ultraviolet bright points: Observations from Solar Orbiter/EUI
DOI: 10.1051/0004-6361/202142884 Bibcode: 2022A&A...662A...7L

Li, Dong

Context. Moving structures have been detected in coronal bright points and in a solar flare in active regions that are bidirectional, symmetrical, simultaneous, and quasi-periodic. These could be regarded as observational evidence of plasma outflows via magnetic reconnection.
Aims: We explored pairs of moving structures in fifteen ultraviolet…

2022 Astronomy and Astrophysics
SolarOrbiter 7
Constraining masses and separations of unseen companions to five accelerating nearby stars
DOI: 10.1051/0004-6361/202244033 Bibcode: 2022A&A...665A..73M

Rouan, D.; Schmidt, T. O. B.; Henning, T. +40 more


Aims: In this work, we aim to constrain the masses and separations of potential substellar companions to five accelerating stars (HIP 1481, HIP 88399, HIP 96334, HIP 30314, and HIP 116063) using multiple data sets acquired with different techniques.
Methods: Our targets were originally observed as part of the SPHERE/SHINE survey, and rad…

2022 Astronomy and Astrophysics
Gaia Hipparcos 7
CHEMOUT: CHEMical complexity in star-forming regions of the OUTer Galaxy. II. Methanol formation at low metallicity
DOI: 10.1051/0004-6361/202243532 Bibcode: 2022A&A...664A.154F

Elia, D.; Magrini, L.; Caselli, P. +8 more

Context. The outer Galaxy is an environment with a lower metallicity than the regions surrounding the Sun and for this reason the formation and survival of molecules in star-forming regions located in the inner and outer Galaxy are expected to be different.
Aims: To gain understanding of how chemistry changes throughout the Milky Way, it is c…

2022 Astronomy and Astrophysics
Herschel 7
Revisiting Ulysses electron data with a triple fit of velocity distributions
DOI: 10.1051/0004-6361/202243477 Bibcode: 2022A&A...663A..67S

Fichtner, H.; Scherer, K.; Lazar, M. +1 more

Context. Given their uniqueness, the Ulysses data can still provide us with valuable new clues about the properties of plasma populations in the solar wind, and especially about their variations with heliographic coordinates. In the context of kinetic waves and instabilities in the solar wind plasma, the electron temperature anisotropy plays a cru…

2022 Astronomy and Astrophysics
Ulysses 7
Evolution of the critical torus instability height and coronal mass ejection likelihood in solar active regions
DOI: 10.1051/0004-6361/202142910 Bibcode: 2022A&A...665A..37J

O'Kane, Jennifer; James, Alexander W.; Williams, David R.


Aims: Working towards improved space weather predictions, we aim to quantify how the critical height at which the torus instability drives coronal mass ejections (CMEs) varies over time in a sample of solar active regions.
Methods: We model the coronal magnetic fields of 42 active regions and quantify the critical height at their central…

2022 Astronomy and Astrophysics
SOHO 7
Establishing the accuracy of asteroseismic mass and radius estimates of giant stars. III. KIC 4054905, an eclipsing binary with two 10 Gyr thick disk RGB stars
DOI: 10.1051/0004-6361/202244345 Bibcode: 2022A&A...668A..82B

Grundahl, F.; Lund, M. N.; Miglio, A. +16 more

Context. Eclipsing binary stars with an oscillating giant component allow accurate stellar parameters to be derived and asteroseismic methods to be tested and calibrated. To this aim, suitable systems need to be firstly identified and secondly measured precisely and accurately. KIC 4054905 is one such system, which has been identified, but with me…

2022 Astronomy and Astrophysics
Gaia 7
Deuteration of c-C3H2 towards the pre-stellar core L1544
DOI: 10.1051/0004-6361/202243422 Bibcode: 2022A&A...664A.119G

Caselli, P.; Spezzano, S.; Sipilä, O. +7 more

Context. In the centre of pre-stellar cores, the deuterium fractionation is enhanced due to the cold temperatures and high densities. Therefore, the chemistry of deuterated molecules can be used to probe the evolution and the kinematics in the earliest stages of star formation.
Aims: We analyse emission maps of cyclopropenylidene, c-C3

2022 Astronomy and Astrophysics
Herschel 7
Searching for anomalous microwave emission in nearby galaxies. K-band observations with the Sardinia Radio Telescope
DOI: 10.1051/0004-6361/202142684 Bibcode: 2022A&A...658L...8B

Bianchi, S.; Madden, S. C.; Galliano, F. +9 more


Aims: We observed four nearby spiral galaxies (NGC 3627, NGC 4254, NGC 4736, and NGC 5055) in the K band with the 64-m Sardinia Radio Telescope, with the aim of detecting anomalous microwave emission (AME), a radiation component presumably due to spinning dust grains, which has been observed thus far in the Milky Way and only in a handful of …

2022 Astronomy and Astrophysics
Herschel 7
THA 15−31: Discovery with VLT/X-shooter and Swift/UVOT of a new symbiotic star of the accreting-only variety
DOI: 10.1051/0004-6361/202142058 Bibcode: 2022A&A...661A.124M

Masetti, N.; Munari, U.; Alcalá, J. M. +4 more

We report the discovery and characterization of a new symbiotic star of the accreting-only variety, which we observed in the optical/near-infrared (NIR) with VLT/X-shooter and in the X-rays/ultraviolet with Swift/UVOT+XRT. The new symbiotic star, THA 15−31, was previously described as a pre-main sequence star belonging to the Lupus 3 association. …

2022 Astronomy and Astrophysics
Gaia 7
SRGA J124404.1-632232/SRGU J124403.8-632231: New X-ray pulsar discovered in the all-sky survey by the SRG
DOI: 10.1051/0004-6361/202141147 Bibcode: 2022A&A...661A..21D

Haberl, F.; Santangelo, A.; Gromadzki, M. +12 more

Ongoing all-sky surveys by the eROSITA and the Mikhail Pavlinsky ART-XC telescopes on board the Spectrum-Roentgen-Gamma (SRG) mission have already revealed over a million of X-ray sources. One of them, SRGA J124404.1-632232/SRGU J124403.8-632231, was detected as a new source in the third (of the planned eight) consecutive X-ray surveys by ART-XC. …

2022 Astronomy and Astrophysics
Gaia 7