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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
Detection of the S(1) Rotational Line of H2 toward IRC+10216: A Simultaneous Measurement of the Mass-loss Rate and CO Abundance
DOI: 10.3847/2041-8213/ac5a58 Bibcode: 2022ApJ...927L..33F

Cernicharo, J.; Fonfría, J. P.; Richter, M. J. +2 more

We report the first detection of the S(1) pure rotational line of ortho-H2 at 17.04 µm in an asymptotic giant branch star, using observations of IRC+10216 with the Echelon-cross-echelle Spectrograph (EXES) mounted on the Stratospheric Observatory for Infrared Astronomy. This line, which was observed in a very high-sensitivity spec…

2022 The Astrophysical Journal
ISO 5
The K2 Galactic Archaeology Program: Overview, target selection, and survey properties
DOI: 10.1093/mnras/stac2031 Bibcode: 2022MNRAS.517.1970S

Bland-Hawthorn, Joss; Sharma, Sanjib; Stello, Dennis +3 more

K2 was a community-driven NASA mission where all targets were proposed through guest observer programmes. Here we provide an overview of one of the largest of these endeavours, the K2 Galactic Archaeology Programme (K2GAP), with about 25 per cent of the observed targets being allocated to this programme. K2GAP provides asteroseismic parameters for…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 5
Spectroscopic and Imaging Observations of Spatially Extended Magnetic Reconnection in the Splitting of a Solar Filament Structure
DOI: 10.3847/2041-8213/ac9dfd Bibcode: 2022ApJ...940L..12H

Liu, Ying D.; Hu, Huidong; Peter, Hardi +2 more

On the Sun, Doppler shifts of bidirectional outflows from the magnetic-reconnection site have been found only in confined regions through spectroscopic observations. Without spatially resolved spectroscopic observations across an extended region, the distribution of reconnection and its outflows in the solar atmosphere cannot be made clear. Magnet…

2022 The Astrophysical Journal
IRIS 5