Search Publications

Searching for Hα-emitting sources in the gaps of five transitional disks. SPHERE/ZIMPOL high-contrast imaging
DOI: 10.1051/0004-6361/202243918 Bibcode: 2022A&A...668A.138H

de Gregorio-Monsalvo, I.; Quanz, S. P.; Montesinos, B. +13 more

Context. (Pre-)Transitional disks show gaps and cavities that can be related to ongoing planet formation. According to theory, young embedded planets can accrete material from the circumplanetary and circumstellar disks and can be detected using accretion tracers, such as the Hα emission line.
Aims: We aim to detect accreting proto…

2022 Astronomy and Astrophysics
Gaia 20
The HD 137496 system: A dense, hot super-Mercury and a cold Jupiter
DOI: 10.1051/0004-6361/202141520 Bibcode: 2022A&A...657A..68A

Bossini, D.; Adibekyan, V.; Hoyer, S. +28 more

Context. Most of the currently known planets are small worlds with radii between that of the Earth and that of Neptune. The characterization of planets in this regime shows a large diversity in compositions and system architectures, with distributions hinting at a multitude of formation and evolution scenarios. However, many planetary populations,…

2022 Astronomy and Astrophysics
Gaia 20
Planet Hunters TESS IV: a massive, compact hierarchical triple star system TIC 470710327
DOI: 10.1093/mnras/stab3619 Bibcode: 2022MNRAS.511.4710E

Aigrain, S.; Lee, S.; Escorza, A. +37 more

We report the discovery and analysis of a massive, compact, hierarchical triple system (TIC 470710327) initially identified by citizen scientists in data obtained by NASA's Transiting Exoplanet Survey Satellite (TESS). Spectroscopic follow-up observations obtained with the HERMES spectrograph, combined with eclipse-timing variations (ETVs), confir…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 20
The Pristine survey - XV. A CFHT ESPaDOnS view on the Milky Way halo and disc populations
DOI: 10.1093/mnras/stab3721 Bibcode: 2022MNRAS.511.1004L

Jablonka, P.; Lardo, C.; Kordopatis, G. +14 more

We present a one-dimensional, local thermodynamic equilibrium homogeneous analysis of 132 stars observed at high resolution with ESPaDOnS. This represents the largest sample observed at high resolution (R ~ 40 000) from the Pristine survey. This sample is based on the first version of the Pristine catalogue and covers the full range of metalliciti…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 20
Cross-checking SMBH mass estimates in NGC 6958 - I. Stellar dynamics from adaptive optics-assisted MUSE observations
DOI: 10.1093/mnras/stab3210 Bibcode: 2022MNRAS.509.5416T

Weilbacher, Peter M.; Krajnović, Davor; van de Ven, Glenn +9 more

Supermassive black hole masses (MBH) can dynamically be estimated with various methods and using different kinematic tracers. Different methods have only been cross-checked for a small number of galaxies and often show discrepancies. To understand these discrepancies, detailed cross-comparisons of additional galaxies are needed. We pres…

2022 Monthly Notices of the Royal Astronomical Society
eHST 20
Magnetic helicity and energy of emerging solar active regions and their erruptivity
DOI: 10.1051/0004-6361/202142868 Bibcode: 2022A&A...662A...6L

Liu, Y.; Nindos, A.; Liokati, E.


Aims: We investigate the role of the accumulation of magnetic helicity and magnetic energy in the generation of coronal mass ejections (CMEs) from emerging solar active regions (ARs).
Methods: Using vector magnetic field data obtained by the Helioseismic and Magnetic Imager on board the Solar Dynamics Observatory, we calculated the magne…

2022 Astronomy and Astrophysics
SOHO 20
The TREX Survey: Kinematical Complexity Throughout M33's Stellar Disk and Evidence for a Stellar Halo
DOI: 10.3847/1538-4357/ac3480 Bibcode: 2022ApJ...924..116G

Williams, Benjamin F.; Gilbert, Karoline M.; Wojno, Jennifer +9 more

We present initial results from a large spectroscopic survey of stars throughout M33's stellar disk. We analyze a sample of 1667 red giant branch (RGB) stars extending to projected distances of ~11 kpc from M33's center (~18 kpc, or ~10 scale lengths, in the plane of the disk). The line-of-sight velocities of RGB stars show the presence of two kin…

2022 The Astrophysical Journal
eHST 19
Absolute Calibration of Cepheid Period-Luminosity Relations in NGC 4258
DOI: 10.3847/1538-4357/ac51db Bibcode: 2022ApJ...940...64Y

Casertano, Stefano; Filippenko, Alexei V.; Riess, Adam G. +6 more

Owing to its accurate distance measured from water-maser motions, NGC 4258 is one of the most important anchors for calibrating the Cepheid period-luminosity relations (PLRs). We expand on previous efforts and carry out a new Cepheid search in this system using the Hubble Space Telescope. We discover and measure a sample of 669 Cepheids in four ne…

2022 The Astrophysical Journal
Gaia eHST 19
Acceleration and cooling of the corona during X-ray flares from the Seyfert galaxy I Zw 1
DOI: 10.1093/mnras/stac416 Bibcode: 2022MNRAS.512..761W

Brandt, W. N.; Costantini, E.; Blandford, R. D. +2 more

We report on X-ray flares that were observed from the active galactic nucleus I Zwicky 1 (I Zw 1) in 2020 January by the NuSTAR and XMM-Newton observatories. The X-ray spectrum is well-described by a model comprised of the continuum emission from the corona and its reflection from the accretion disc around a rapidly spinning (a > 0.94) black ho…

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 19
Completeness of the Gaia verse - V. Astrometry and radial velocity sample selection functions in Gaia EDR3
DOI: 10.1093/mnras/stab3262 Bibcode: 2022MNRAS.509.6205E

Everall, Andrew; Boubert, Douglas

We risk reaching false scientific conclusions if we test our physical theories against subsets of the Gaia catalogue without correcting for the biased process by which stars make it into our sample. In this paper, we produce selection functions for three Gaia science samples to enable the community to correct for this bias. We estimate the probabi…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 19