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MAGAZ3NE: High Stellar Velocity Dispersions for Ultramassive Quiescent Galaxies at z ≳ 3
DOI: 10.3847/1538-4357/ac8747 Bibcode: 2022ApJ...938..109F

Cooper, M. C.; Urbano Stawinski, Stephanie M.; Muzzin, Adam +17 more

In this work, we publish stellar velocity dispersions, sizes, and dynamical masses for eight ultramassive galaxies (UMGs; $\mathrm{log}({M}_{* }/{M}_{\odot })$ > 11), z ≳ 3) from the Massive Ancient Galaxies At z > 3 NEar-infrared (MAGAZ3NE) Survey, more than doubling the number of such galaxies with velocity dispersion measurements at this …

2022 The Astrophysical Journal
eHST 26
New Coronae and Stellar Associations Revealed by a Clustering Analysis of the Solar Neighborhood
DOI: 10.3847/1538-4357/ac8c25 Bibcode: 2022ApJ...939...94M

Faherty, Jacqueline K.; Gagné, Jonathan; Moranta, Leslie +1 more

We present the results of a density-based clustering analysis of the 6D XYZ Galactic positions and UVW-space velocities of nearby (≤200 pc) Gaia Early Data Release 3 stars with radial velocities using HDBSCAN, in opposition to previous studies (Kounkel & Covey 2019; Meingast et al. 2021) that only included positions and tangential velocities. …

2022 The Astrophysical Journal
Gaia 26
WO-type Wolf-Rayet Stars: The Last Hurrah of Massive Star Evolution
DOI: 10.3847/1538-4357/ac66e7 Bibcode: 2022ApJ...931..157A

Aadland, Erin; Massey, Philip; Hillier, D. John +3 more

Are WO-type Wolf-Rayet (WR) stars in the final stage of massive star evolution before core-collapse? Although WC- and WO-type WRs have very similar spectra, WOs show a much stronger O VI λλ3811,34 emission-line feature. This has usually been interpreted to mean that WOs are more oxygen rich than WCs, and thus further evolved. However, previous stu…

2022 The Astrophysical Journal
eHST 25
Constraining the Physical Properties of Stellar Coronal Mass Ejections with Coronal Dimming: Application to Far-ultraviolet Data of ϵ Eridani
DOI: 10.3847/1538-4357/ac80c1 Bibcode: 2022ApJ...936..170L

Loyd, R. O. Parke; France, Kevin; Youngblood, Allison +9 more

Coronal mass ejections (CMEs) are a prominent contributor to solar system space weather and might have impacted the Sun's early angular momentum evolution. A signal diagnostic of CMEs on the Sun is coronal dimming: a drop in coronal emission, tied to the mass of the CME, that is the direct result of removing emitting plasma from the corona. We pre…

2022 The Astrophysical Journal
SOHO eHST 25
A New Method for Direct Measurement of Isotopologue Ratios in Protoplanetary Disks: A Case Study of the 12CO/13CO Ratio in the TW Hya Disk
DOI: 10.3847/1538-4357/ac6efb Bibcode: 2022ApJ...932..126Y

Nomura, Hideko; Tsukagoshi, Takashi; Furuya, Kenji +2 more

Planetary systems are thought to be born in protoplanetary disks. Isotope ratios are a powerful tool for investigating the material origin and evolution from molecular clouds to planetary systems via protoplanetary disks. However, it is challenging to measure the isotope (isotopologue) ratios, especially in protoplanetary disks, because the emissi…

2022 The Astrophysical Journal
Gaia 25
The First Near-infrared Transmission Spectrum of HIP 41378 f, A Low-mass Temperate Jovian World in a Multiplanet System
DOI: 10.3847/2041-8213/ac559d Bibcode: 2022ApJ...927L...5A

Kirk, James; López-Morales, Mercedes; Alam, Munazza K. +22 more

We present a near-infrared transmission spectrum of the long-period (P = 542 days), temperate (T eq = 294 K) giant planet HIP 41378 f obtained with the Wide-Field Camera 3 instrument aboard the Hubble Space Telescope (HST). With a measured mass of 12 ± 3 M and a radius of 9.2 ± 0.1 R , HIP 41378 f has an extreme…

2022 The Astrophysical Journal
eHST 25
A Census of Optically Dark Massive Galaxies in the Early Universe from Magnification by Lensing Galaxy Clusters
DOI: 10.3847/1538-4357/ac3de5 Bibcode: 2022ApJ...926..155S

Kong, Xu; Zheng, Wei; Liu, Daizhong +10 more

We present ALMA 870 µm and JCMT/SCUBA2 850 µm dust continuum observations of a sample of optically dark and strongly lensed galaxies in cluster fields. The ALMA and SCUBA2 observations reach a median rms of ~0.11 mJy and 0.44 mJy, respectively, with the latter close to the confusion limit of the data at 850 µm. This represents on…

2022 The Astrophysical Journal
eHST 25
Extragalactic Magnetism with SOFIA (SALSA Legacy Program). IV. Program Overview and First Results on the Polarization Fraction
DOI: 10.3847/1538-4357/ac7f9d Bibcode: 2022ApJ...936...92L

Reach, William T.; Dale, Daniel A.; Lopez-Rodriguez, Enrique +12 more

We present the first data release of the Survey on extragALactic magnetiSm with SOFIA (SALSA Legacy Program) with a set of 14 nearby (<20 Mpc) galaxies with resolved imaging polarimetric observations using HAWC+ from 53 to 214 µm at a resolution of 5″-18″ (90 pc-1 kpc). We introduce the definitions of and background on extragalactic magne…

2022 The Astrophysical Journal
Herschel 25
Changing-look Event in NGC 3516: Continuum or Obscuration Variability?
DOI: 10.3847/1538-4357/ac42ca Bibcode: 2022ApJ...925...84M

Brenneman, Laura W.; Kriss, Gerard A.; Mehdipour, Missagh +6 more

The Seyfert-1 galaxy NGC 3516 has undergone major spectral changes in recent years. In 2017 we obtained Chandra, NuSTAR, and Swift observations during its new low-flux state. Using these observations, we model the spectral energy distribution (SED) and the intrinsic X-ray absorption, and compare the results with those from historical observations …

2022 The Astrophysical Journal
XMM-Newton 25
The Physical Properties of the SVS 13 Protobinary System: Two Circumstellar Disks and a Spiraling Circumbinary Disk in the Making
DOI: 10.3847/1538-4357/ac3b50 Bibcode: 2022ApJ...930...91D

Ho, Paul T. P.; Zapata, Luis A.; Carrasco-González, Carlos +13 more

We present Very Large Array (VLA) and Atacama Large Millimeter/submillimeter Array (ALMA) observations of the close (0.″3 = 90 au separation) protobinary system SVS 13. We detect two small circumstellar disks (radii ~12 and ~9 au in dust, and ~30 au in gas) with masses of ~0.004-0.009 M for VLA 4A (the western component) and ~0.009-0.…

2022 The Astrophysical Journal
Gaia 25