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Signatures of strong magnetization and a metal-poor atmosphere for a Neptune-sized exoplanet
DOI: 10.1038/s41550-021-01505-x Bibcode: 2022NatAs...6..141B

Mikal-Evans, Thomas; Sing, David K.; López-Morales, Mercedes +10 more

The magnetosphere of an exoplanet has yet to be unambiguously detected. Investigations of star-planet interaction and neutral atomic hydrogen absorption during transit to detect magnetic fields in hot Jupiters have been inconclusive, and interpretations of the transit absorption non-unique. In contrast, ionized species escaping a magnetized exopla…

2022 Nature Astronomy
XMM-Newton eHST 51
Multiple Channels for the Onset of Magnetism in Isolated White Dwarfs
DOI: 10.3847/2041-8213/ac84d3 Bibcode: 2022ApJ...935L..12B

Landstreet, John D.; Bagnulo, Stefano

The presence of a strong magnetic field is a feature common to a significant fraction of degenerate stars, yet little is understood about the field's origin and evolution. New observational constraints from volume-limited surveys point to a more complex situation than a single mechanism valid for all stars. We show that in high-mass white dwarfs, …

2022 The Astrophysical Journal
Gaia 51
GOALS-JWST: Tracing AGN Feedback on the Star-forming Interstellar Medium in NGC 7469
DOI: 10.3847/2041-8213/ac9ebf Bibcode: 2022ApJ...941L..36L

Inami, Hanae; Böker, Torsten; Law, David R. +34 more

We present James Webb Space Telescope (JWST) Mid-Infrared Instrument (MIRI) integral-field spectroscopy of the nearby merging, luminous infrared galaxy, NGC 7469. This galaxy hosts a Seyfert type-1.5 nucleus, a highly ionized outflow, and a bright, circumnuclear star-forming ring, making it an ideal target to study active galactic nucleus (AGN) fe…

2022 The Astrophysical Journal
AKARI JWST 51
Early Results from GLASS-JWST. I: Confirmation of Lensed z ≥ 7 Lyman-break Galaxies behind the Abell 2744 Cluster with NIRISS
DOI: 10.3847/2041-8213/ac8e6e Bibcode: 2022ApJ...938L..13R

Santini, Paola; Castellano, Marco; Fontana, Adriano +29 more

We present the first search for z ≥ 7, continuum-confirmed Lyman break sources with NIRISS/WFS spectroscopy over the Abell 2744 Frontier Fields cluster, as part of the GLASS-JWST-ERS survey. With ~15 hr of preimaging and multiangle grism exposures in the F115W, F150W, and F200W filters, we describe the general data handling (i.e., reduction, clean…

2022 The Astrophysical Journal
eHST JWST 51
Classifying Be Star Variability With TESS. I. The Southern Ecliptic
DOI: 10.3847/1538-3881/ac5abd Bibcode: 2022AJ....163..226L

Labadie-Bartz, Jonathan; Carciofi, Alex C.; Henrique de Amorim, Tajan +4 more

TESS photometry is analyzed for 430 classical Be stars observed in the first year of the mission. The often complex and diverse variability of each object in this sample is classified to obtain an understanding of the behavior of this class as a population. Ninety-seven percent of the systems are variable above the noise level, with timescales spa…

2022 The Astronomical Journal
Gaia 50
Asteroid taxonomy from cluster analysis of spectrometry and albedo
DOI: 10.1051/0004-6361/202243587 Bibcode: 2022A&A...665A..26M

Carry, B.; Mahlke, M.; Mattei, P. -A.

Context. The classification of the minor bodies of the Solar System based on observables has been continuously developed and iterated over the past 40 yr. While prior iterations followed either the availability of large observational campaigns or new instrumental capabilities opening new observational dimensions, we see the opportunity to improve …

2022 Astronomy and Astrophysics
AKARI 50
A major asymmetric ice trap in a planet-forming disk. III. First detection of dimethyl ether
DOI: 10.1051/0004-6361/202142981 Bibcode: 2022A&A...659A..29B

Booth, Alice S.; van Dishoeck, Ewine F.; Nazari, Pooneh +3 more

The complex organic molecules (COMs) detected in star-forming regions are the precursors of the prebiotic molecules that can lead to the emergence of life. By studying COMs in more evolved protoplanetary disks we can gain a better understanding of how they are incorporated into planets. This paper presents ALMA band 7 observations of the dust and …

2022 Astronomy and Astrophysics
Gaia 50
Distance estimates for AGB stars from parallax measurements
DOI: 10.1051/0004-6361/202243670 Bibcode: 2022A&A...667A..74A

De Beck, E.; Ramstedt, S.; Vlemmings, W. H. T. +1 more

Context. Estimating the distances to asymptotic giant branch (AGB) stars using optical measurements of their parallaxes is not straightforward because of the large uncertainties introduced by their dusty envelopes, their large angular sizes, and their surface brightness variability.
Aims: This paper aims to assess the reliability of the dista…

2022 Astronomy and Astrophysics
Gaia 50
Data Release 2 of S-PLUS: Accurate template-fitting based photometry covering 1000 deg2 in 12 optical filters
DOI: 10.1093/mnras/stac284 Bibcode: 2022MNRAS.511.4590A

Molino, A.; Werle, A.; Mendes de Oliveira, C. +32 more

The Southern Photometric Local Universe Survey (S-PLUS) is an ongoing survey of ~9300 deg2 in the southern sky in a 12-band photometric system. This paper presents the second data release (DR2) of S-PLUS, consisting of 514 tiles covering an area of 950 deg2. The data has been fully calibrated using a new photometric calibrati…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 50
The R-process Alliance: A Nearly Complete R-process Abundance Template Derived from Ultraviolet Spectroscopy of the R-process-enhanced Metal-poor Star HD 222925
DOI: 10.3847/1538-4365/ac5cbc Bibcode: 2022ApJS..260...27R

Beers, Timothy C.; Placco, Vinicius M.; Hattori, Kohei +9 more

We present a nearly complete rapid neutron-capture process (r-process) chemical inventory of the metal-poor ([Fe/H] = -1.46 ± 0.10) r-process-enhanced ([Eu/Fe] = +1.32 ± 0.08) halo star HD 222925. This abundance set is the most complete for any object beyond the solar system, with a total of 63 metals detected and seven with upper limits. It compr…

2022 The Astrophysical Journal Supplement Series
Gaia eHST 50