Search Publications

Toward the true number of flaring giant stars in the Kepler field. Are their flaring specialities associated with their being giant stars?
DOI: 10.1051/0004-6361/202039674 Bibcode: 2021A&A...647A..62O

Pál, A.; Günther, M. N.; Oláh, K. +4 more


Aims: We aim to give a reliable estimate of the number of flaring giant stars in the Kepler field. By analyzing the flaring activity of these stars, we explored their flare statistics and the released flare energies. The role of oscillation in suppressing magnetic activity was also investigated. We searched for flaring specialities that may b…

2021 Astronomy and Astrophysics
Gaia 15
The HARPS search for southern extra-solar planets. XLVI. 12 super-Earths around the solar type stars HD 39194, HD 93385, HD 96700, HD 154088, and HD 189567
DOI: 10.1051/0004-6361/202141351 Bibcode: 2021A&A...654A.104U

Alonso, R.; Bouchy, F.; Deleuil, M. +23 more

Context. We present precise radial-velocity measurements of five solar-type stars observed with the HARPS Echelle spectrograph mounted on the 3.6-m telescope in La Silla (ESO, Chile). With a time span of more than 10 yr and a fairly dense sampling, the survey is sensitive to low mass planets down to super-Earths on orbital periods up to 100 days. …

2021 Astronomy and Astrophysics
Gaia 14
Solar surges related to UV bursts. Characterization through k-means, inversions, and density diagnostics
DOI: 10.1051/0004-6361/202141472 Bibcode: 2021A&A...655A..28N

Guglielmino, S. L.; Sainz Dalda, A.; Nóbrega-Siverio, D.

Context. Surges are cool and dense ejections typically observed in chromospheric lines and closely related to other solar phenomena such as UV bursts or coronal jets. Even though surges have been observed for decades now, questions regarding their fundamental physical properties such as temperature and density, as well as their impact on upper lay…

2021 Astronomy and Astrophysics
IRIS 14
Characterizing the morphology of the debris disk around the low-mass star GSC 07396-00759
DOI: 10.1051/0004-6361/202140740 Bibcode: 2021A&A...653A..88A

Bayo, A.; Ginski, C.; Henning, Th. +17 more

Context. Debris disks have commonly been studied around intermediate-mass stars. Their intense radiation fields are believed to efficiently remove the small dust grains that are constantly replenished by collisions. For lower-mass central objects, in particular M stars, the dust removal mechanism needs to be further investigated given the much wea…

2021 Astronomy and Astrophysics
Gaia XMM-Newton 14
Water and methanol ice in L 1544
DOI: 10.1051/0004-6361/201936385 Bibcode: 2021A&A...651A..53G

Alves, J.; Caselli, P.; Jiménez-Serra, I. +4 more

Context. Methanol and complex organic molecules have been found in cold starless cores, where a standard warm-up scenario would not work because of the absence of heat sources. A recent chemical model attributed the presence of methanol and large organics to the efficient chemical desorption and a class of neutral-neutral reactions that proceed fa…

2021 Astronomy and Astrophysics
Herschel 14
The reduced proper motion selected halo: Methods and description of the catalogue
DOI: 10.1051/0004-6361/202038178 Bibcode: 2021A&A...645A..69K

Helmi, Amina; Koppelman, Helmer H.

Context. The Gaia mission has provided the largest ever astrometric chart of the Milky Way. Using it to map the Galactic halo is helpful for disentangling its merger history.
Aims: The identification of halo stars in Gaia DR2 with reliable distance estimates requires special methods because such stars are typically farther away and scarce.

2021 Astronomy and Astrophysics
Gaia 14
Three faint-source microlensing planets detected via the resonant-caustic channel
DOI: 10.1051/0004-6361/202141517 Bibcode: 2021A&A...655A..21H

Han, Cheongho; Udalski, Andrzej; Lee, Chung-Uk +32 more


Aims: We conducted a project of reinvestigating the 2017-2019 microlensing data collected by high-cadence surveys with the aim of finding planets that were missed due to the deviations of planetary signals from the typical form of short-term anomalies.
Methods: The project led us to find three planets, KMT-2017-BLG-2509Lb, OGLE-2017-BLG-…

2021 Astronomy and Astrophysics
eHST 14
Blue extreme disk-runaway stars with Gaia EDR3
DOI: 10.1051/0004-6361/202040178 Bibcode: 2021A&A...646L...4I

Raddi, Roberto; Irrgang, Andreas; Heber, Ulrich +1 more

Since the discovery of hypervelocity stars in 2005, it has been widely believed that only the disruption of a binary system by a supermassive black hole at the Galactic center (GC), that is, the so-called Hills mechanism, is capable of accelerating stars to beyond the Galactic escape velocity. In the meantime, however, driven by the Gaia space mis…

2021 Astronomy and Astrophysics
Gaia 14
Atacama Cosmology Telescope measurements of a large sample of candidates from the Massive and Distant Clusters of WISE Survey. Sunyaev-Zeldovich effect confirmation of MaDCoWS candidates using ACT
DOI: 10.1051/0004-6361/202141200 Bibcode: 2021A&A...653A.135O

Hilton, Matt; Sifón, Cristóbal; Choi, Steve K. +35 more

Context. Galaxy clusters are an important tool for cosmology, and their detection and characterization are key goals for current and future surveys. Using data from the Wide-field Infrared Survey Explorer (WISE), the Massive and Distant Clusters of WISE Survey (MaDCoWS) located 2839 significant galaxy overdensities at redshifts 0.7 ≲ z ≲ 1.5, whic…

2021 Astronomy and Astrophysics
Herschel 14
The MUSE Hubble Ultra Deep Field Survey. XVI. The angular momentum of low-mass star-forming galaxies: A cautionary tale and insights from TNG50
DOI: 10.1051/0004-6361/202040225 Bibcode: 2021A&A...654A..49B

Bacon, Roland; Contini, Thierry; Richard, Johan +14 more

We investigate the specific angular momentum (sAM) j(< r) profiles of intermediate redshift (0.4 < z < 1.4) star-forming galaxies (SFGs) in the relatively unexplored regime of low masses (down to M ∼ 108 M) and small sizes (down to Re ∼ 1.5 kpc), and we characterize the sAM scaling relation (i…

2021 Astronomy and Astrophysics
eHST 14