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The ALMA-ALPAKA survey. I. High-resolution CO and [CI] kinematics of star-forming galaxies at z = 0.5-3.5
DOI: 10.1051/0004-6361/202346444 Bibcode: 2023A&A...679A.129R

Magdis, G. E.; Zanella, A.; Brammer, G. +13 more

Context. Spatially resolved studies of the kinematics of galaxies provide crucial insights into their assembly and evolution, enabling one to infer the properties of the dark matter halos, derive the impact of feedback on the interstellar medium (ISM), as well as measure and characterize the outflow motions. To date, most of the kinematic studies …

2023 Astronomy and Astrophysics
eHST 37
Gaia white dwarfs within 40 pc - III. Spectroscopic observations of new candidates in the Southern hemisphere
DOI: 10.1093/mnras/stac3303 Bibcode: 2023MNRAS.518.3055O

Hermes, J. J.; Gänsicke, B. T.; Jordan, S. +31 more

We present a spectroscopic survey of 248 white dwarf candidates within 40 pc of the Sun; of these 244 are in the Southern hemisphere. Observations were performed mostly with the Very Large Telescope (X-Shooter) and Southern Astrophysical Research Telescope. Almost all candidates were selected from Gaia Data Release 3 (DR3). We find a total of 246 …

2023 Monthly Notices of the Royal Astronomical Society
Gaia 37
PHANGS-JWST First Results: Massive Young Star Clusters and New Insights from JWST Observations of NGC 1365
DOI: 10.3847/2041-8213/acae94 Bibcode: 2023ApJ...944L..14W

White, Richard L.; Henshaw, Jonathan D.; Kruijssen, J. M. Diederik +28 more

A primary new capability of JWST is the ability to penetrate the dust in star-forming galaxies to identify and study the properties of young star clusters that remain embedded in dust and gas. In this Letter we combine new infrared images taken with JWST with our optical Hubble Space Telescope (HST) images of the starbursting barred (Seyfert2) spi…

2023 The Astrophysical Journal
eHST JWST 37
Waves in the lower solar atmosphere: the dawn of next-generation solar telescopes
DOI: 10.1007/s41116-022-00035-6 Bibcode: 2023LRSP...20....1J

Stangalini, Marco; Jess, David B.; Jafarzadeh, Shahin +3 more

Waves and oscillations have been observed in the Sun's atmosphere for over half a century. While such phenomena have readily been observed across the entire electromagnetic spectrum, spanning radio to gamma-ray sources, the underlying role of waves in the supply of energy to the outermost extremities of the Sun's corona has yet to be uncovered. Of…

2023 Living Reviews in Solar Physics
SOHO 37
Stellar Properties of Observed Stars Stripped in Binaries in the Magellanic Clouds
DOI: 10.3847/1538-4357/ace5a3 Bibcode: 2023ApJ...959..125G

Smith, N.; Crowther, P. A.; de Mink, S. E. +6 more

Massive stars (~8-25 M ) stripped of their hydrogen-rich envelopes via binary interaction are thought to be the main progenitors for merging neutron stars and stripped-envelope supernovae. We recently presented the discovery of the first set of such stripped stars in a companion paper. Here, we fit the spectra of 10 stars with new atmo…

2023 The Astrophysical Journal
Gaia 37
Internal kinematics of Gaia DR3 wide binaries: anomalous behaviour in the low acceleration regime
DOI: 10.1093/mnras/stad2306 Bibcode: 2023MNRAS.525.1401H

Hernandez, X.

The Gaia eDR3 catalogue has recently been used to study statistically the internal kinematics of wide binary populations using relative velocities of the two component stars, ΔV, total binary masses, mB, and separations, s. For s ≳ 0.01 pc, these binaries probe the low-acceleration a ≲ 2a0 regime where gravitational anomalies…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 37
Empirical Temperature- and Extinction-dependent Extinction Coefficients for the GALEX, Pan-STARRS 1, Gaia, SDSS, 2MASS, and WISE Passbands
DOI: 10.3847/1538-4365/ac9dfa Bibcode: 2023ApJS..264...14Z

Yuan, Haibo; Zhang, Ruoyi

We have obtained accurate dust reddening from the far-ultraviolet to the mid-infrared for up to 5 million stars by the star-pair algorithm based on LAMOST stellar parameters along with Galaxy Evolution Explorer, Pan-STARRS 1, Gaia, Sloan Digital Sky Survey, Two Micron All Sky Survey, and Wide-field Infrared Survey Explorer photometric data. The ty…

2023 The Astrophysical Journal Supplement Series
Gaia 37
The Puzzling Properties of the MACS1149-JD1 Galaxy at z = 9.11
DOI: 10.3847/2041-8213/ad0159 Bibcode: 2023ApJ...957L..18S

Stiavelli, Massimo; Treu, Tommaso; Trenti, Michele +6 more

We analyze new JWST NIRCam and NIRSpec data on the redshift 9.11 galaxy MACS1149-JD1 (hereafter JD1). Our NIRCam imaging data reveal that JD1 comprises three spatially distinct components. Our spectroscopic data indicate that JD1 appears dust free but is already enriched, $12+\mathrm{log}({\rm{O}}/{\rm{H}})={7.90}_{-0.05}^{+0.04}$ . We also find t…

2023 The Astrophysical Journal
eHST JWST 37
Using [Ne V]/[Ne III] to Understand the Nature of Extreme-ionization Galaxies
DOI: 10.3847/1538-4357/acde55 Bibcode: 2023ApJ...953...10C

Papovich, Casey; Finkelstein, Steven L.; Cleri, Nikko J. +14 more

Spectroscopic studies of extreme-ionization galaxies (EIGs) are critical to our understanding of exotic systems throughout cosmic time. These EIGs exhibit spectral features requiring >54.42 eV photons: the energy needed to ionize helium into He2+ fully and emit He II recombination lines. Spectroscopic studies of EIGs can probe exotic…

2023 The Astrophysical Journal
eHST JWST 37
The hidden side of cosmic star formation at z > 3. Bridging optically dark and Lyman-break galaxies with GOODS-ALMA
DOI: 10.1051/0004-6361/202245100 Bibcode: 2023A&A...672A..18X

Magnelli, B.; Daddi, E.; Elbaz, D. +37 more

Our current understanding of the cosmic star formation history at z > 3 is primarily based on UV-selected galaxies (Lyman-break galaxies, i.e., LBGs). Recent studies of H-dropouts (HST-dark galaxies) have revealed that we may be missing a large proportion of star formation that is taking place in massive galaxies at z > 3. In this work, we e…

2023 Astronomy and Astrophysics
Herschel eHST 37