Search Publications

Evolution of the Sun's activity and the poleward transport of remnant magnetic flux in Cycles 21-24
DOI: 10.1093/mnras/stab3528 Bibcode: 2022MNRAS.510.1331M

Banerjee, Dipankar; Karak, Bidya Binay; Kumar, Pawan +4 more

Detailed study of the solar magnetic field is crucial to understand its generation, transport, and reversals. The timing of the reversals may have implications on space weather and thus identification of the temporal behaviour of the critical surges that lead to the polar field reversals is important. We analyse the evolution of solar activity and…

2022 Monthly Notices of the Royal Astronomical Society
SOHO 25
New Craters on Mars: An Updated Catalog
DOI: 10.1029/2021JE007145 Bibcode: 2022JGRE..12707145D

Piqueux, S.; Dundas, C. M.; Werynski, A. +15 more

We present a catalog of new impacts on Mars. These craters formed in the last few decades, constrained with repeat orbital imaging. Crater diameters range from 58 m down to <1 m. For each impact, we report whether it formed a single crater or a cluster (58% clusters); albedo features of the blast zone (88% halos; 64% linear rays; 10% arcuate ra…

2022 Journal of Geophysical Research (Planets)
MEx 25
The COMBS Survey - III. The chemodynamical origins of metal-poor bulge stars
DOI: 10.1093/mnras/stab2878 Bibcode: 2022MNRAS.509..122L

Kobayashi, Chiaki; Hawkins, Keith; Lucey, Madeline +6 more

The characteristics of the stellar populations in the Galactic bulge inform and constrain the Milky Way's formation and evolution. The metal-poor population is particularly important in light of cosmological simulations, which predict that some of the oldest stars in the Galaxy now reside in its centre. The metal-poor bulge appears to consist of m…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 25
Linking stellar populations to H II regions across nearby galaxies. I. Constraining pre-supernova feedback from young clusters in NGC 1672
DOI: 10.1051/0004-6361/202243766 Bibcode: 2022A&A...662L...6B

Boquien, M.; Chevance, M.; Dale, D. A. +32 more

Context. Stellar feedback is one of the fundamental factors regulating the evolution of galaxies. However, we still do not have access to strong observational constraints on the relative importance of the different feedback mechanisms (e.g. radiation, ionised gas pressure, stellar winds) in driving H II region evolution and molecular cloud disrupt…

2022 Astronomy and Astrophysics
eHST 25
The Spectroscopic Binaries from the LAMOST Medium-resolution Survey. I. Searching for Double-lined Spectroscopic Binaries with a Convolutional Neural Network
DOI: 10.3847/1538-4365/ac42d1 Bibcode: 2022ApJS..258...26Z

Tian, Hao; Ji, Xin; Zong, Weikai +13 more

We developed a convolutional neural network model to distinguish the double-lined spectroscopic binaries (SB2s) from others based on single-exposure medium-resolution spectra (R ~ 7500). The training set consists of a large set of mock spectra of single stars and binaries synthesized based on the MIST stellar evolutionary model and ATLAS9 atmosphe…

2022 The Astrophysical Journal Supplement Series
Gaia 25
The resolved scaling relations in DustPedia: Zooming in on the local Universe
DOI: 10.1051/0004-6361/202245043 Bibcode: 2022A&A...668A.130C

Clark, Christopher J. R.; Mosenkov, Aleksandr V.; Baes, Maarten +18 more


Aims: We perform a homogeneous analysis of an unprecedented set of spatially resolved scaling relations (SRs) between interstellar medium (ISM) components, that is to say dust, gas, and gas-phase metallicity, and other galaxy properties, such as stellar mass (Mstar), total baryonic content, and star-formation rate (SFR), in a range…

2022 Astronomy and Astrophysics
Herschel 25
Untangling the Galaxy. IV. Empirical Constraints on Angular Momentum Evolution and Gyrochronology for Young Stars in the Field
DOI: 10.3847/1538-3881/ac866d Bibcode: 2022AJ....164..137K

Stassun, Keivan G.; Kounkel, Marina; Bouma, Luke G. +3 more

We present a catalog of ~100,000 periodic variable stars in Transiting Exoplanet Survey Satellite (TESS) full-frame image data among members of widely distributed moving groups identified with Gaia in the previous papers in the series. By combining the periods from our catalog attributable to rotation with previously derived rotation periods for b…

2022 The Astronomical Journal
Gaia 25
A census of X-ray millisecond pulsars in globular clusters
DOI: 10.1093/mnras/stac442 Bibcode: 2022MNRAS.511.5964Z

Zhao, Jiaqi; Heinke, Craig O.

We present a comprehensive census of X-ray millisecond pulsars (MSPs) in 29 Galactic globular clusters (GCs), including 68 MSPs with confirmed X-ray luminosities and 107 MSPs with X-ray upper limits. We compile previous X-ray studies of GC MSPs, and add new analyses of six MSPs (PSRs J1326-4728A, J1326-4728B, J1518+0204C, J1717+4308A, J1737-0314A,…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 25
The complex stellar system M 22: confirming abundance variations with high precision differential measurements
DOI: 10.1093/mnras/stac2254 Bibcode: 2022MNRAS.516.3515M

Milone, A. P.; Marino, A. F.; Legnardi, M. V. +8 more

M 22 (NGC 6656) is a chemically complex globular cluster-like system reported to harbour heavy element abundance variations. However, the extent of these variations and the origin of this cluster is still debated. In this work, we investigate the chemical in-homogeneity of M 22 using differential line-by-line analysis of high-quality (R = 110 000,…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 25
Monochromatic Globular Clusters as a Critical Test of Formation Models for the Dark Matter-deficient Galaxies NGC 1052-DF2 and NGC 1052-DF4
DOI: 10.3847/2041-8213/ac94d6 Bibcode: 2022ApJ...940L...9V

van Dokkum, Pieter; Romanowsky, Aaron J.; Conroy, Charlie +8 more

It was recently proposed that the dark matter-deficient ultradiffuse galaxies DF2 and DF4 in the NGC 1052 group could be the products of a "bullet dwarf" collision between two gas-rich progenitor galaxies. In this model, DF2 and DF4 formed at the same time in the immediate aftermath of the collision, and a strong prediction is that their globular …

2022 The Astrophysical Journal
eHST 25