Search Publications

Smoke on the wind: dust nucleation in the archetype colliding-wind pinwheel WR 104
DOI: 10.1093/mnras/stac2999 Bibcode: 2023MNRAS.518.3211S

Millour, F.; Lau, R. M.; Soulain, A. +2 more

A handful of binary Wolf-Rayet stars are known to harbour spectacular spiral structures spanning a few hundred astronomical units. These systems host some of the highest dust production rates in the Universe and are therefore interesting candidates for addressing the origin of the enigmatic dust excess observed across galactic evolution. The subst…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 4
An XMM-Newton View of the Andromeda Galaxy as Explored in a Legacy Survey (New-ANGELS). I. The X-Ray Source Catalog
DOI: 10.3847/1538-4365/ace4b8 Bibcode: 2023ApJS..268...36H

Bregman, Joel N.; Zhang, Yi; Wang, Q. Daniel +6 more

We introduce the New-ANGELS program, an XMM-Newton survey of a ~7.2 deg2 area around M31, which aims to study the X-ray populations in the M31 disk and the X-ray-emitting hot gas in the inner halo of M31 up to 30 kpc. In this first paper, we report the catalog of 4506 detected X-ray sources and attempt to cross-identify or roughly class…

2023 The Astrophysical Journal Supplement Series
Gaia XMM-Newton 4
Kinetic Alfvén Waves Excited by Multiple Free Energy Sources in the Magnetotail
DOI: 10.3847/1538-4357/acd11a Bibcode: 2023ApJ...951...53B

Lakhina, G. S.; Singh, S. V.; Barik, K. C.

The generation of kinetic Alfvén waves (KAWs) is investigated through a three-component theoretical model incorporating ion beam and velocity shear as the sources of free energy in a non-Maxwellian κ-distributed plasmas. The model considers Maxwellian distributed background ions, drifting-Maxwellian beam ions, and κ-electrons as its constituent sp…

2023 The Astrophysical Journal
Cluster 4
Examining the Properties of Low-luminosity Hosts of Type Ia Supernovae from ASAS-SN
DOI: 10.3847/1538-4357/acce35 Bibcode: 2023ApJ...950..108H

Galbany, L.; Morrell, Nidia; Holoien, Thomas W. -S. +14 more

We present a spectroscopic analysis of 44 low-luminosity host galaxies of Type Ia supernovae (SNe Ia) detected by the All-Sky Automated Survey for Supernovae (ASAS-SN), using hydrogen, oxygen, and sulfur emission lines to measure metallicities and star formation rates. We find no statistically significant evidence that the star formation activity …

2023 The Astrophysical Journal
Gaia 4
No plateau observed in late-time near-infrared observations of the underluminous Type Ia supernova 2021qvv
DOI: 10.1093/mnras/stad2960 Bibcode: 2023MNRAS.526.2977G

Galbany, L.; Rest, A.; Howell, D. A. +23 more

Near-infrared (NIR) observations of normal Type Ia supernovae (SNe Ia) obtained between 150 and 500 d past maximum light reveal the existence of an extended plateau. Here, we present observations of the underluminous, 1991bg-like SN 2021qvv. Early, ground-based optical and NIR observations show that SN 2021qvv is similar to SN 2006mr, making it on…

2023 Monthly Notices of the Royal Astronomical Society
eHST 4
Spatially Resolved Recent Star Formation History in NGC 6946
DOI: 10.3847/1538-4357/aced44 Bibcode: 2023ApJ...954..211T

Dolphin, Andrew; Telford, O. Grace; Koplitz, Brad +6 more

The nearby face-on star-forming spiral galaxy NGC 6946 is known as the Fireworks Galaxy due to its hosting an unusually large number of supernovae. We analyze its resolved near-ultraviolet stellar photometry measured from images taken with the Hubble Space Telescope's Wide Field Camera 3 with the F275W and F336W filters. We model the color-magnitu…

2023 The Astrophysical Journal
Gaia eHST 4
A rotational age for the open cluster NGC 2281. The possibility of using the fast rotator sequence for accurate cluster age determinations
DOI: 10.1051/0004-6361/202346083 Bibcode: 2023A&A...674A.152F

Strassmeier, K. G.; Granzer, T.; Barnes, S. A. +3 more

Context. Cool star rotation periods have become an important tool in determining ages of open clusters.
Aims: We aim to estimate the age of the open cluster NGC 2281 based on the rotational properties of its low-mass members. Previous age estimates for this open cluster range from 275 Myr to 630 Myr.
Methods: Based on an eight month-long…

2023 Astronomy and Astrophysics
Gaia 4
Radio multiwavelength analysis of the compact disk CX Tau: Presence of strong free-free variability or anomalous microwave emission
DOI: 10.1051/0004-6361/202347042 Bibcode: 2023A&A...677A.118C

Lodato, G.; Testi, L.; Tazzari, M. +8 more

Protoplanetary disks emit radiation across a broad range of wavelengths, requiring a multiwavelength approach to fully understand their physical mechanisms and how they form planets. Observations at submillimeter to centimeter wavelengths can provide insights into the thermal emission from dust, free-free emission from ionized gas, and possible gy…

2023 Astronomy and Astrophysics
Gaia 4
Chronology, composition, and mineralogy of mare basalts in the junction of Oceanus Procellarum, Mare Imbrium, Mare Insularum, and Mare Vaporum
DOI: 10.1016/j.icarus.2023.115531 Bibcode: 2023Icar..39715531Z

Chen, Jian; Zhao, Zixu; Ling, Zongcheng +2 more

The timeline of volcanic activity is critical for constraining the thermal evolution of the Moon. The spatial extents of mare basalts, major products of lunar volcanism, have been precisely extracted from LROC (Lunar Reconnaissance Orbiter Camera) image mosaics. With the maria extents newly extracted from LROC mosaics, we found that a large area o…

2023 Icarus
Chandrayaan-1 4
A Lithium Depletion Age for the Carina Association
DOI: 10.3847/1538-3881/ad03f3 Bibcode: 2023AJ....166..247W

Kraus, Adam L.; Barber, Madyson G.; Mann, Andrew W. +6 more

The dispersed remnants of stellar nurseries, stellar associations, provide unparalleled samples of coeval stars critical for studies of stellar and planetary formation and evolution. The Carina Stellar Association is one of the closest stellar associations to Earth, and yet measurements of its age have varied from 13 to 45 Myr. We aim to update th…

2023 The Astronomical Journal
Gaia 4