Search Publications

Statistics of BY Draconis chromospheric variable stars
DOI: 10.1093/mnras/stac1660 Bibcode: 2022MNRAS.514.4932C

de Grijs, Richard; Kamath, Devika; Chen, Xiaodian +1 more

We present an extensive catalogue of BY Draconis (BY Dra)-type variables and their stellar parameters. BY Dra are main-sequence FGKM-type stars. They exhibit inhomogeneous starspots and bright faculae in their photospheres. These features are caused by stellar magnetic fields, which are carried along with the stellar disc through rotation and whic…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 5
High-contrast, high-angular resolution view of the GJ 367 exoplanet system
DOI: 10.1093/mnras/stac961 Bibcode: 2022MNRAS.513..661B

Brandner, Wolfgang; Calissendorff, Per; Cantalloube, Faustine +1 more

We search for additional companions in the GJ 367 exoplanet system and aim to better constrain its age and evolutionary status. We analyse high-contrast direct imaging observations obtained with HST/NICMOS, VLT/NACO, and VLT/SPHERE. We investigate and critically discuss conflicting age indicators based on theoretical isochrones and models for Gala…

2022 Monthly Notices of the Royal Astronomical Society
Gaia eHST 5
Peculiar hydrogen-deficient carbon stars: strontium-rich stars and the s-process
DOI: 10.1051/0004-6361/202142882 Bibcode: 2022A&A...667A..85C

Clayton, Geoffrey C.; Tisserand, Patrick; Crawford, Courtney L. +1 more

Context. R Coronae Borealis (RCB) variables and their non-variable counterparts, the dustless Hydrogen-deficient Carbon (dLHdC) stars have been known to exhibit enhanced s-processed material on their surfaces, especially Sr, Y, and Ba. No comprehensive work has been done to explore the s-process in these types of stars, however one particular RCB …

2022 Astronomy and Astrophysics
Gaia 5
Chemically Peculiar Stars in the Open Cluster Stock 2
DOI: 10.3847/1538-3881/ac9c56 Bibcode: 2022AJ....164..255C

Bouy, Hervé; Agüeros, Marcel A.; Gebran, Marwan +2 more

The recently rediscovered open cluster Stock 2, located roughly 375 pc away and about 400 Myr old, has the potential to be an exciting new testbed for our understanding of stellar evolution. We present results from a spectroscopic campaign to characterize stars near the cluster's main-sequence turnoff; our goal is to identify candidate chemically …

2022 The Astronomical Journal
Gaia 5
Galactic Cosmic Rays at Mars and Venus: Temporal Variations from Hours to Decades Measured as the Background Signal of Onboard Microchannel Plates
DOI: 10.3847/1538-4357/ac9a49 Bibcode: 2022ApJ...940..178F

Barabash, Stas; Nilsson, Hans; Holmström, Mats +8 more

A microchannel plate (MCP) is a component widely used for counting particles in space. Using the background counts from MCPs on the Mars Express and Venus Express orbiters-operating over 17 yr and 8 yr, respectively-we investigated the galactic cosmic ray (GCR) characteristics of the inner solar system. The MCP background counts at Mars and Venus,…

2022 The Astrophysical Journal
MEx VenusExpress 5
Evidence of globular cluster abundance anomalies in the SMC intermediate-age cluster Kron 3
DOI: 10.1093/mnras/stac1724 Bibcode: 2022MNRAS.515.2511S

Da Costa, G. S.; Milone, A. P.; Marino, A. F. +5 more

Using spectra obtained with the VLT/FORS2 and Gemini-S/GMOS-S instruments, we have investigated carbon, nitrogen, and sodium abundances in a sample of red giant members of the Small Magellanic Cloud star cluster Kron 3. The metallicity and luminosity of the cluster are comparable to those of Galactic globular clusters but it is notably younger (ag…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 5
Ionization and Star Formation in the Giant H II Region SMC-N66
DOI: 10.1088/1538-3873/ac697b Bibcode: 2022PASP..134f4301G

Kniazev, A.; Hamann, W. -R.; Sabbi, E. +8 more

The NGC 346 young stellar system and associated N66 giant H II region in the Small Magellanic Cloud are the nearest example of a massive star-forming event in a low metallicity (Z ≈ 0.2Z ) galaxy. With an age of ≲3 Myr this system provides a unique opportunity to study relationships between massive stars and their associated H II regio…

2022 Publications of the Astronomical Society of the Pacific
eHST 5
Constraining Europa's Subsolar Atmosphere With a Joint Analysis of HST Spectral Images and Galileo Magnetic Field Data
DOI: 10.1029/2022JA030472 Bibcode: 2022JGRA..12730472C

Saur, J.; Cervantes, S.

We constrain Europa's tenuous atmosphere on the subsolar hemisphere by combining two sets of observations: oxygen emissions at 1,304 and 1,356 Å from Hubble Space Telescope (HST) spectral images and Galileo magnetic field measurements from its closest encounter, the E12 flyby. We describe Europa's atmosphere with three neutral gas species: global …

2022 Journal of Geophysical Research (Space Physics)
eHST 5
CaSSIS-based stereo products for Mars after three years in orbit
DOI: 10.1016/j.pss.2022.105515 Bibcode: 2022P&SS..21905515R

Mège, Daniel; Pajola, Maurizio; Cremonese, Gabriele +10 more

The Colour and Stereo Surface Imaging System (CaSSIS) on board the ExoMars Trace Gas Orbiter (TGO), operating in push-frame mode, provides multiband images at four different wavelengths thanks to a Filter Strip Assembly with a panchromatic filter and three broadband filters within the visible and near infrared range. The camera acquires stereo pai…

2022 Planetary and Space Science
ExoMars-16 5
Upstream solar wind speed at comet 67P. Reconstruction method, model comparison, and results
DOI: 10.1051/0004-6361/202142867 Bibcode: 2022A&A...659A..18N

Holmström, M.; Gunell, H.; Futaana, Y. +7 more

Context. Rosetta followed comet 67P at heliocentric distances from 1.25 to 3.6 au. The solar wind was observed for much of this time, but was significantly deflected and to some extent slowed down by the interaction with the coma.
Aims: We use the different changes in the speed of H+ and He2+ when they interact with the …

2022 Astronomy and Astrophysics
MEx Rosetta 5