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Survey for distant solar twins (SDST) - II. Design, observations, and data
DOI: 10.1093/mnras/stac3033 Bibcode: 2022MNRAS.517.5569L

Kos, Janez; Martell, Sarah L.; Murphy, Michael T. +5 more

Studies of solar twins have key impacts on the astronomical community, but only ~100-200 nearby solar twins (<1 kpc) have been reliably identified over the last few decades. The aim of our survey (SDST) is to identify ~150-200 distant solar twins and analogues (up to ≲4 kpc) closer to the Galactic Centre. We took advantage of the precise Gaia a…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 2
Scattering and sublimation: a multiscale view of µm-sized dust in the inclined disc of HD 145718
DOI: 10.1093/mnras/stac149 Bibcode: 2022MNRAS.511.2434D

Monnier, John D.; Schaefer, Gail H.; Lanthermann, Cyprien +16 more

We present multi-instrument observations of the disc around the Herbig Ae star, HD 145718, employing geometric and Monte Carlo radiative transfer models to explore the disc orientation, the vertical and radial extent of the near-infrared (NIR) scattering surface, and the properties of the dust in the disc surface and sublimation rim. The disc appe…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 2
Brighter and More Massive Galaxies in the Vicinity of Lyα Nebulae
DOI: 10.3847/1538-4357/aca3ac Bibcode: 2022ApJ...941..180W

Wells, Natalie K.; Prescott, Moire K. M.; Finlator, Kristian M.

It has been well established in the local universe that galaxy properties differ based on the large-scale environment in which they reside. As luminous Lyα nebulae have been shown to trace overdense environments at z ~ 2-3, comparing the properties of galaxies within Lyα nebulae systems to those in the field can provide insight into how and when l…

2022 The Astrophysical Journal
eHST 2
Discrete Element Modeling of Aeolian-like Morphologies on Comet 67P/Churyumov-Gerasimenko
DOI: 10.1051/0004-6361/202141296 Bibcode: 2022A&A...662A...2S

Otto, K. A.; Sachse, M.; Kappel, D. +1 more

Context. Even after the Rosetta mission, some of the mechanical parameters of comet 67P/Churyumov-Gerasimenko's surface material are still not well constrained. They are needed to improve our understanding of cometary activity or for planning sample return procedures.
Aims: We discuss the physical process dominating the formation of aeolian-l…

2022 Astronomy and Astrophysics
Rosetta 2
Joint Survey Processing. II. Stellar Proper Motions in the COSMOS Field from Hubble Space Telescope ACS and Subaru Telescope HSC Observations
DOI: 10.3847/1538-4357/ac5a4f Bibcode: 2022ApJ...930...71F

Fajardo-Acosta, Sergio B.; Faisst, Andreas; Grillmair, Carl J. +4 more

We analyze stellar proper motions in the COSMOS field to assess the presence of bulk motions. At bright magnitudes (G-band 18.5-20.76 AB), we use the proper motions of 1010 stars in the Gaia DR2 catalog. At the faint end, we compute proper motions of 11,519 pointlike objects at i-band magnitudes 19-25 AB using Hubble ACS and Subaru HSC data, which…

2022 The Astrophysical Journal
Gaia eHST 2
Color Dependence of the Transit Detectability of Young Active M Dwarfs
DOI: 10.3847/1538-3881/ac937d Bibcode: 2022AJ....164..209M

Gaidos, Eric; Miyakawa, Kohei; Hirano, Teruyuki +2 more

We investigate the planetary transit detectability in the presence of stellar rotational activity from light curves of young M dwarfs, and estimate the improvements in detection at near-infrared (NIR) wavelengths. By making maps of the transit signal detection efficiency over the orbital period and planetary radius with light curves of the members…

2022 The Astronomical Journal
Gaia 2
Multi-scale image preprocessing and feature tracking for remote CME characterization
DOI: 10.1051/swsc/2022020 Bibcode: 2022JSWSC..12...20S

Stepanyuk, Oleg; Kozarev, Kamen; Nedal, Mohamed

Coronal Mass Ejections (CMEs) influence the interplanetary environment over vast distances in the solar system by injecting huge clouds of fast solar plasma and energetic particles (SEPs). A number of fundamental questions remain about how SEPs are produced, but current understanding points to CME-driven shocks and compressions in the solar corona…

2022 Journal of Space Weather and Space Climate
SolarOrbiter 2
Solid confirmation of the broad DIB around 864.8 nm using stacked Gaia-RVS spectra
DOI: 10.1051/0004-6361/202244343 Bibcode: 2022A&A...666L..12Z

Schultheis, M.; Marshall, D. J.; Smith, M. +26 more

Context. Studies of the correlation between different diffuse interstellar bands (DIBs) are important for exploring their origins. However, the Gaia-RVS spectral window between 846 and 870 nm contains few DIBs, the strong DIB at 862 nm being the only convincingly confirmed one.
Aims: Here we attempt to confirm the existence of a broad DIB aro…

2022 Astronomy and Astrophysics
Gaia 2
Assessment of the accuracy of measures in the 1829 southern double star catalogue of James Dunlop
DOI: 10.1093/mnras/stab3777 Bibcode: 2022MNRAS.510.5330L

Letchford, Roderick R.; White, Graeme L.; Brown, Carolyn J.

In 1829 James Dunlop published the first southern double star catalogue of some 253 double stars. The accuracy of this catalogue has been determined by using Aladin to cross-match them with Gaia DR2 and estimate their positional (right ascension, declination, position angle, and separation) and magnitude accuracy. Seven per cent could not be ident…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 2
Polarimetric Studies of a Fast Coronal Mass Ejection
DOI: 10.1007/s11207-022-02018-0 Bibcode: 2022SoPh..297...78M

Bemporad, Alessandro; Mierla, Marilena; Inhester, Bernd +4 more

In this work we performed a polarimetric study of a fast and wide coronal mass ejection (CME) observed on 12 July 2012 by the COR1 and COR2 instruments onboard the Solar TErrestrial RElations Observatory (STEREO) mission. The CME source region was an X1.4 flare located at approximately S15W01 on the solar disk, as observed from the Earth's perspec…

2022 Solar Physics
SOHO 2