Search Publications

Atmospheric processes affecting methane on Mars
DOI: 10.1016/j.icarus.2022.114940 Bibcode: 2022Icar..38214940G

Rauer, H.; Arnold, G.; Herbst, K. +6 more

It is currently uncertain as to whether methane exists on Mars. Data from the Curiosity Rover suggests a background methane concentration of a few tenths parts per billion whereas data from the Trace Gas Orbiter suggest an upper limit of twenty parts per trillion. If methane exists on Mars then we do not understand fully the physical and chemical …

2022 Icarus
ExoMars-16 6
Probing the megaparsec-scale environment of hyperluminous infrared galaxies at 2 < z < 4
DOI: 10.1051/0004-6361/202244072 Bibcode: 2022A&A...668A..54G

Wang, L.; Farrah, D.; Clements, D. +3 more

Context. Protoclusters are progenitors of galaxy clusters and they serve as an important key in studies of how halo mass and stellar mass assemble in the early universe. Finding the signposts of such overdense regions, such as bright dusty star-forming galaxies (DSFG), is a popular method for identifying protocluster candidates.
Aims: Hyperlu…

2022 Astronomy and Astrophysics
Herschel 6
A machine learning approach to photometric metallicities of giant stars
DOI: 10.1093/mnras/stac2550 Bibcode: 2022MNRAS.516.5521F

Sanders, Jason L.; Fallows, Connor P.

Despite the advances provided by large-scale photometric surveys, stellar features - such as metallicity - generally remain limited to spectroscopic observations often of bright, nearby low-extinction stars. To rectify this, we present a neural network approach for estimating the metallicities and distances of red giant stars with 8-band photometr…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 6
GRB 190919B: Rapid optical rise explained as a flaring activity
DOI: 10.1051/0004-6361/202143010 Bibcode: 2022A&A...662A.126J

Karpov, Sergey; Hu, Y. -D.; Castro-Tirado, Alberto J. +17 more

Following the detection of a long GRB 190919B by INTEGRAL (INTErnational Gamma-Ray Astrophysics Laboratory), we obtained an optical photometric sequence of its optical counterpart. The light curve of the optical emission exhibits an unusually steep rise ∼100 s after the initial trigger. This behaviour is not expected from a `canonical' GRB optical…

2022 Astronomy and Astrophysics
INTEGRAL 6
Probing the innermost region of the AU Microscopii debris disc
DOI: 10.1051/0004-6361/202244226 Bibcode: 2022A&A...665A..41G

Milli, J.; Boccaletti, A.; Girard, J. H. +5 more

Context. AU Mic is a young and nearby M-dwarf star harbouring a circumstellar debris disc and one recently discovered planet on an eight-day orbit. Large-scale structures within the disc were also discovered and are moving outwards at high velocity.
Aims: We aim to study this system with the highest spatial resolution in order to probe the in…

2022 Astronomy and Astrophysics
Gaia 6
No globular cluster progenitors in Milky Way satellite galaxies
DOI: 10.1093/mnras/stac2578 Bibcode: 2022MNRAS.516.4560B

Bovy, Jo; Boldrini, Pierre

In order to find the possible progenitors of Milky Way (MW) globular clusters, we perform orbit integrations to track the orbits of 170 Galactic globular clusters and the 11 classical MW satellite galaxies backwards in time for 11 Gyr in an MW-plus-satellites potential including the response of the MW to the infall of the Large Magellanic Cloud an…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 6
CoSHA: Code for Stellar Properties Heuristic Assignment-for the MaStar Stellar Library
DOI: 10.3847/1538-4365/ac67f4 Bibcode: 2022ApJS..261...20M

Yan, Renbin; Drory, Niv; Bruzual, Gustavo +5 more

We introduce COSHA: a Code for Stellar properties Heuristic Assignment. In order to estimate the stellar properties, COSHA implements a Gradient Tree Boosting algorithm to label each star across the parameter space (T eff, $\mathrm{log}g$ , [Fe/H], and [α/Fe]). We use COSHA to estimate the stellar atmospheric parameters of 22,000 unique…

2022 The Astrophysical Journal Supplement Series
Gaia 6
Probing the shape of the Milky Way dark matter halo with hypervelocity stars: A new method
DOI: 10.1051/0004-6361/202142679 Bibcode: 2022A&A...663A..72G

Gallo, Arianna; Ostorero, Luisa; Chakrabarty, Sankha Subhra +2 more

We propose a new method for determining the shape of the gravitational potential of the dark matter (DM) halo of the Milky Way (MW) with the galactocentric tangential velocities of a sample of hypervelocity stars (HVSs). We compute the trajectories of different samples of HVSs in a MW where the baryon distribution is axisymmetric and the DM potent…

2022 Astronomy and Astrophysics
Gaia 6
Relationships Between the Spectra of Near-Earth Proton Enhancements, Hard X-Ray Bursts, and CME Speeds
DOI: 10.1007/s11207-022-01986-7 Bibcode: 2022SoPh..297...53K

Grechnev, V. V.; Kiselev, V. I.; Meshalkina, N. S.

Some studies propose the transfer of flare-accelerated protons in an erupting flux rope until its reconnection with an open structure releases the trapped protons. Coulomb collisions in the dense flux-rope body deplete the low-energy part of the proton spectrum. On the other hand, shock acceleration progressively replenishes this part of the spect…

2022 Solar Physics
SOHO 6
The escape of globular clusters from the satellite dwarf galaxies of the Milky Way
DOI: 10.1093/mnras/stac1070 Bibcode: 2022MNRAS.513.3526R

Haghi, Hosein; Zonoozi, Akram Hasani; Khalaj, Pouria +2 more

Using numerical simulations, we have studied the escape of globular clusters (GCs) from the satellite dwarf spheroidal galaxies (dSphs) of the Milky Way (MW). We start by following the orbits of a large sample of GCs around dSphs in the presence of the MW potential field. We then obtain the fraction of GCs leaving their host dSphs within a Hubble …

2022 Monthly Notices of the Royal Astronomical Society
Gaia 6