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ALMA-LEGUS. II. The Influence of Subgalactic Environments on Molecular Cloud Properties
DOI: 10.3847/1538-4357/ad198a Bibcode: 2024ApJ...964...13F

Grebel, Eva K.; Smith, Linda J.; Aloisi, Alessandra +24 more

We compare the molecular cloud properties in subgalactic regions of two galaxies, barred spiral NGC 1313, which is forming many massive clusters, and flocculent spiral NGC 7793, which is forming significantly fewer massive clusters despite having a similar star formation rate to NGC 1313. We find that there are larger variations in cloud propertie…

2024 The Astrophysical Journal
eHST 4
Spatially correlated stellar accretion in the Lupus star-forming region: Evidence for ongoing infall from the interstellar medium
DOI: 10.1051/0004-6361/202452120 Bibcode: 2024A&A...691A.169W

Benisty, Myriam; Manara, Carlo F.; Gupta, Aashish +1 more

Context. Growing evidence suggests that protoplanetary discs may be influenced by late stage infall from the interstellar medium (ISM). It remains unclear the degree to which infall shapes disc populations at ages ≳1 Myr. Aims. We explored possible spatial correlations between stellar accretion rates in the Lupus star-forming region, which would s…

2024 Astronomy and Astrophysics
Gaia 4
Braving the Storm: Quantifying Disk-wide Ionized Outflows in the Large Magellanic Cloud with ULLYSES
DOI: 10.3847/1538-4357/ad64d2 Bibcode: 2024ApJ...974...22Z

Choi, Yumi; Olsen, Knut; Roman-Duval, Julia +11 more

The Large Magellanic Cloud (LMC) is home to many H II regions, which may lead to significant outflows. We examine the LMC's multiphase gas (T∼104-5 K) in H I, S II, Si IV, and C IV using 110 stellar sight lines from the Hubble Space Telescope's Ultraviolet Legacy Library of Young Stars as Essential Standards program. We develop a contin…

2024 The Astrophysical Journal
eHST 4
Migration and Evolution of giant ExoPlanets (MEEP). I. Nine Newly Confirmed Hot Jupiters from the TESS Mission
DOI: 10.3847/1538-3881/ad4a57 Bibcode: 2024AJ....168...32S

Lester, Kathryn V.; Bieryla, Allyson; Latham, David W. +72 more

Hot Jupiters were many of the first exoplanets discovered in the 1990s, but in the decades since their discovery the mysteries surrounding their origins have remained. Here we present nine new hot Jupiters (TOI-1855 b, TOI-2107 b, TOI-2368 b, TOI-3321 b, TOI-3894 b, TOI-3919 b, TOI-4153 b, TOI-5232 b, and TOI-5301 b) discovered by NASA's TESS miss…

2024 The Astronomical Journal
Gaia 4
Three super-Earths and a possible water world from TESS and ESPRESSO
DOI: 10.1051/0004-6361/202450505 Bibcode: 2024A&A...688A.216H

Bouchy, F.; Rebolo, R.; Allende Prieto, C. +52 more

Context. Since 2018, the ESPRESSO spectrograph at the VLT has been hunting for planets in the southern skies via the radial velocity (RV) method. One of its goals is to follow up on candidate planets from transit surveys such as the TESS mission, with a particular focus on small planets for which ESPRESSO's RV precision is vital.
Aims: We aim…

2024 Astronomy and Astrophysics
Gaia 4
JWST View of Four Infant Galaxies at z = 8.31–8.49 in the MACS J0416.1‑2403 Field and Implications for Reionization
DOI: 10.3847/1538-4357/ad7b32 Bibcode: 2024ApJ...975...87M

Grogin, Norman A.; Hathi, Nimish P.; Koekemoer, Anton M. +35 more

New JWST/NIRCam wide-field slitless spectroscopy provides redshifts for four z > 8 galaxies located behind the lensing cluster MACS J0416.1‑2403. Two of them, "Y1" and "JD," have previously reported spectroscopic redshifts based on Atacama Large Millimeter/submillimeter Array measurements of [O III] 88 µm and/or [C II] 157.7 µm line…

2024 The Astrophysical Journal
eHST JWST 4
The Molecular Clouds of M31
DOI: 10.3847/1538-4357/ad38bf Bibcode: 2024ApJ...966..193L

Forbrich, Jan; Lada, Charles J.; Petitpas, Glen +1 more

Deep interferometric observations of CO and dust continuum emission are obtained with the Submillimeter Array at 230 GHz to investigate the physical nature of the giant molecular cloud (GMC) population in the Andromeda galaxy (M31). We use J = 2 ‑ 1 12CO and 13CO emission to derive the masses, sizes, and velocity dispersions …

2024 The Astrophysical Journal
Herschel 4
Characterization of the δ Scuti eclipsing binary KIC 4851217 and its tertiary companion as well as detection of tidally tilted pulsations
DOI: 10.1093/mnras/stae1879 Bibcode: 2024MNRAS.533.2705J

Handler, G.; Southworth, J.; Kurtz, D. W. +3 more

Stellar theory enables us to understand the properties of stars at different stages of their evolution, and contributes to other fields of astrophysics such as galactic and exoplanet studies. Assessing the accuracy of stellar theories necessitates high precision, model-independent measurements of the properties of real stars, such as those obtaina…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 4
Deeper than DEEP: a spectroscopic survey of z > 3 Ly α emitters in the Extended Groth Strip
DOI: 10.1093/mnras/stae361 Bibcode: 2024MNRAS.528.5624U

Finkelstein, Steven L.; Pérez-González, Pablo G.; Bagley, Micaela B. +13 more

We present a spectroscopic survey of Ly α emitters in the Extended Groth Strip (EGS) field, targeting the regime near the Epoch of Reionization. Using Keck/DEep Imaging Multi-Object Spectrograph, we observed 947 high-z candidates with photometric redshifts from 3 < zphot < 7 and down to an H-band (Hubble Space Telescope/Wide Field…

2024 Monthly Notices of the Royal Astronomical Society
eHST JWST 4
Decomposing the AIA 304 Å Channel into Its Cool and Hot Components
DOI: 10.1007/s11207-024-02337-4 Bibcode: 2024SoPh..299...94A

Antolin, Patrick; Auchère, Frédéric; Soubrié, Elie +2 more

The AIA 304 Å channel on board the Solar Dynamics Observatory (SDO) offers a unique view of ≈105 K plasma emitting in the He II 304 Å line. However, when observing off-limb, the emission of the (small) cool structures in the solar atmosphere (such as spicules, coronal rain and prominence material) can be of the same order as the surrounding hot co…

2024 Solar Physics
IRIS 4