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The Physical Parameters of Four WC-type Wolf-Rayet Stars in the Large Magellanic Cloud: Evidence of Evolution
DOI: 10.3847/1538-4357/ac3426 Bibcode: 2022ApJ...924...44A

Aadland, Erin; Massey, Philip; Hillier, D. John +1 more

We present a spectral analysis of four Large Magellanic Cloud (LMC) WC-type Wolf-Rayet (WR) stars (BAT99-8, BAT99-9, BAT99-11, and BAT99-52) to shed light on two evolutionary questions surrounding massive stars. The first is: are WO-type WR stars more oxygen enriched than WC-type stars, indicating further chemical evolution, or are the strong high…

2022 The Astrophysical Journal
eHST 11
Spectroscopic Orbits of Subsystems in Multiple Stars. VIII.
DOI: 10.3847/1538-3881/ac5330 Bibcode: 2022AJ....163..161T

Tokovinin, Andrei

Periods, eccentricities, and masses in hierarchical stellar systems inform us on the formation and early evolution of these fascinating objects. To complement the multiplicity statistics of nearby solar-type stars, 19 new spectroscopic orbits of inner subsystems in 15 hierarchies (10 triples and 5 quadruples) are determined based on high-resolutio…

2022 The Astronomical Journal
Gaia 11
New Insights Into Subsurface Stratigraphy Northwest of Ascraeus Mons, Mars, Using the SHARAD and MARSIS Radar Sounders
DOI: 10.1029/2022JE007210 Bibcode: 2022JGRE..12707210S

Plaut, J. J.; Carter, L. M.; Morgan, G. A. +2 more

The Tharsis Montes volcanoes on Mars are the source of laterally extensive lava flows and other volcanic deposits generating a complex stratigraphy throughout the Tharsis Volcanic Province. We use SHAllow RADar (SHARAD) and Mars Advanced Radar for Subsurface and Ionospheric Sounding (MARSIS) observations in a region northwest of Ascraeus Mons to d…

2022 Journal of Geophysical Research (Planets)
MEx 11
[C II] Map of the Molecular Ring and Arms of the Spiral Galaxy NGC 7331
DOI: 10.3847/1538-4357/ac4252 Bibcode: 2022ApJ...926...82S

Fadda, Dario; Sutter, Jessica

We present the [C II] 157.7 µm map of galaxy NGC 7331 obtained with the Field-Imaging Far-Infrared Line Spectrometer on board the Stratospheric Observatory for Infrared Astronomy (SOFIA). This map extends an existent Herschel/Photodetector Array Camera and Spectrometer observation of the central strip of the galaxy to encompass the entire mo…

2022 The Astrophysical Journal
Herschel ISO 11
The APEX Large CO Heterodyne Orion Legacy Survey (ALCOHOLS). I. Survey overview
DOI: 10.1051/0004-6361/201937034 Bibcode: 2022A&A...658A.178S

Smith, M. D.; Eislöffel, J.; Williams, J. P. +29 more

Context. The Orion molecular cloud complex harbours the nearest Giant Molecular Clouds (GMCs) and the nearest site of high-mass star formation. Its young star and protostar populations are thoroughly characterized. The region is therefore a prime target for the study of star formation.
Aims: Here, we verify the performance of the SuperCAM 64 …

2022 Astronomy and Astrophysics
Herschel 11
A warm super-Neptune around the G-dwarf star TOI-1710 revealed with TESS, SOPHIE, and HARPS-N
DOI: 10.1051/0004-6361/202143002 Bibcode: 2022A&A...666A.183K

Deleuil, M.; Moutou, C.; Carmona, A. +50 more

We report the discovery and characterization of the transiting extrasolar planet TOI-1710 b. It was first identified as a promising candidate by the Transiting Exoplanet Survey Satellite. Its planetary nature was then established with SOPHIE and HARPS-N spectroscopic observations via the radial-velocity method. The stellar parameters for the host …

2022 Astronomy and Astrophysics
Gaia 11
Student Dust Counter Status Report: The First 50 au
DOI: 10.3847/PSJ/ac5ab7 Bibcode: 2022PSJ.....3...69B

Singer, Kelsi N.; James, David; Weaver, Harold +12 more

The Venetia Burney Student Dust Counter (SDC) is an in situ dust detector on board the New Horizons spacecraft measuring the interplanetary dust particle (IDP) distribution for grains with mass m > 10-12 g. SDC provides a near-continuous measure of the interplanetary dust environment, with recent results spanning beyond 50 au. This c…

2022 The Planetary Science Journal
Ulysses 11
Melnick 33Na: a very massive colliding-wind binary system in 30 Doradus
DOI: 10.1093/mnras/stab3521 Bibcode: 2022MNRAS.510.6133B

Townsley, Leisa K.; Broos, Patrick S.; Crowther, Paul A. +2 more

We present spectroscopic analysis of the luminous X-ray source Melnick 33Na (Mk 33Na, HSH95 16) in the Large Magellanic Cloud (LMC) 30 Doradus region (Tarantula Nebula), utilizing new time-series Very Large Telescope/Ultraviolet and Visual Echelle Spectrograph spectroscopy. We confirm Mk 33Na as a double-lined O-type spectroscopic binary with a ma…

2022 Monthly Notices of the Royal Astronomical Society
Gaia eHST 11
Joint Survey Processing. I. Compact Oddballs in the COSMOS Field-Low-luminosity Quasars at z > 6?
DOI: 10.3847/1538-4357/ac59b3 Bibcode: 2022ApJ...929...66F

Koekemoer, Anton M.; Brammer, Gabriel; Miyatake, Hironao +8 more

The faint-end slope of the quasar luminosity function at z ~ 6 and its implication on the role of quasars in reionizing the intergalactic medium at early times has been an outstanding problem for some time. The identification of faint high-redshift quasars with luminosities of <1044.5 erg s-1 is challenging. They are rare …

2022 The Astrophysical Journal
eHST 11
Observations of Instability-driven Nanojets in Coronal Loops
DOI: 10.3847/1538-4357/ac7870 Bibcode: 2022ApJ...934..190S

Antolin, Patrick; McLaughlin, James A.; Sukarmadji, A. Ramada C.

The recent discovery of nanojets by Antolin et al. represents magnetic reconnection in a braided field, thus clearly identifying reconnection-driven nanoflares. Due to their small scale (500 km in width, 1500 km in length) and short timescales (<15 s), it is unclear how pervasive nanojets are in the solar corona. In this paper, we present Inter…

2022 The Astrophysical Journal
IRIS 11