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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
The discovery of rest-frame UV colour gradients and a diversity of dust morphologies in bright z ≃ 7 Lyman-break galaxies
DOI: 10.1093/mnras/stab3744 Bibcode: 2022MNRAS.510.5088B

Bowler, R. A. A.; Cullen, F.; McLure, R. J. +2 more

We present deep ALMA dust continuum observations for a sample of luminous (MUV < -22) star-forming galaxies at z ≃ 7. We detect five of the six sources in the far-infrared (FIR), providing key constraints on the obscured star formation rate (SFR) and the infrared-excess-β (IRX-β) relation without the need for stacking. Despite the ga…

2022 Monthly Notices of the Royal Astronomical Society
eHST 50
NGC 5846-UDG1: A Galaxy Formed Mostly by Star Formation in Massive, Extremely Dense Clumps of Gas
DOI: 10.3847/2041-8213/ac590a Bibcode: 2022ApJ...927L..28D

van Dokkum, Pieter; Romanowsky, Aaron J.; Conroy, Charlie +10 more

It has been shown that ultra-diffuse galaxies (UDGs) have higher specific frequencies of globular clusters, on average, than other dwarf galaxies with similar luminosities. The UDG NGC 5846-UDG1 is among the most extreme examples of globular cluster-rich galaxies found so far. Here we present new Hubble Space Telescope observations and analysis of…

2022 The Astrophysical Journal
eHST 50
Fast plasmoid-mediated reconnection in a solar flare
DOI: 10.1038/s41467-022-28269-w Bibcode: 2022NatCo..13..640Y

Feng, Xueshang; Song, Yongliang; Xue, Zhike +8 more

Magnetic reconnection is a multi-faceted process of energy conversion in astrophysical, space and laboratory plasmas that operates at microscopic scales but has macroscopic drivers and consequences. Solar flares present a key laboratory for its study, leaving imprints of the microscopic physics in radiation spectra and allowing the macroscopic evo…

2022 Nature Communications
Hinode 50
Sizes of Lensed Lower-luminosity z = 4-8 Galaxies from the Hubble Frontier Field Program
DOI: 10.3847/1538-4357/ac4791 Bibcode: 2022ApJ...927...81B

Oesch, P. A.; Bouwens, R. J.; Illingworth, G. D. +3 more

We constrain the rest-UV size-luminosity relation for star-forming galaxies at z ~ 4 and z ~ 6, 7, and 8 identified behind clusters from the Hubble Frontier Fields (HFF) program. The size-luminosity relation is key to deriving accurate luminosity functions (LF) for faint galaxies. Making use of the latest lensing models and full data set for these…

2022 The Astrophysical Journal
eHST 49
Determination of X-ray pulsar geometry with IXPE polarimetry
DOI: 10.1038/s41550-022-01799-5 Bibcode: 2022NatAs...6.1433D

Wu, Kinwah; Enoto, Teruaki; Turolla, Roberto +91 more

Using observations of X-ray pulsar Hercules X-1 by the Imaging X-ray Polarimetry Explorer we report a highly significant (>17σ) detection of the polarization signal from an accreting neutron star. The observed degree of linear polarization of ~10% is far below theoretical expectations for this object, and stays low throughout the spin cycle of …

2022 Nature Astronomy
Gaia 49
Implications for galaxy formation models from observations of globular clusters around ultra-diffuse galaxies
DOI: 10.1093/mnras/stac328 Bibcode: 2022MNRAS.511.4633S

Beasley, Michael A.; Trujillo, Ignacio; Peletier, Reynier F. +5 more

We present an analysis of Hubble Space Telescope observations of globular clusters (GCs) in six ultradiffuse galaxies (UDGs) in the Coma cluster, a sample that represents UDGs with large effective radii (Re), and use the results to evaluate competing formation models. We eliminate two significant sources of systematic uncertainty in the…

2022 Monthly Notices of the Royal Astronomical Society
eHST 49
Planetary Nebulae: Sources of Enlightenment
DOI: 10.1088/1538-3873/ac32b1 Bibcode: 2022PASP..134b2001K

Henry, R. B. C.; Kwitter, Karen B.

In this review/tutorial we explore planetary nebulae as a stage in the evolution of low-to-intermediate-mass stars, as major contributors to the mass and chemical enrichment of the interstellar medium, and as astrophysical laboratories. We discuss many observed properties of planetary nebulae, placing particular emphasis on element abundance deter…

2022 Publications of the Astronomical Society of the Pacific
Gaia 49