Search Publications

Wind-line Variability and Intrinsic Errors in Observational Mass-loss Rates
DOI: 10.3847/1538-4357/ad5440 Bibcode: 2024ApJ...971..166M

Massa, Derck; Oskinova, Lidia M.; Prinja, Raman K.

UV wind-line variability in OB stars appears to be universal. In order to quantify this variation and to estimate its effect on a mass-loss rate determined from a single observation, we use the International Ultraviolet Explorer archive to identify nonpeculiar OB stars with well-developed but unsaturated Si IV λ1400 doublets and at least 10 indepe…

2024 The Astrophysical Journal
Gaia IUE 2
Pre-impact Thermophysical Properties and the Yarkovsky Effect of NASA DART Target (65803) Didymos
DOI: 10.3847/PSJ/ad23eb Bibcode: 2024PSJ.....5...66R

Kolb, Ulrich C.; Daly, R. Terik; Rivkin, Andrew S. +8 more

The NASA Double Asteroid Redirection Test (DART) spacecraft impacted the secondary body of the binary asteroid (65803) Didymos on 2022 September 26 and altered its orbit about the primary body. Before the DART impact, we performed visible and mid-infrared observations to constrain the pre-impact thermophysical properties of the Didymos system and …

2024 The Planetary Science Journal
JWST 2
The April 2023 SYM-H = −233 nT Geomagnetic Storm: A Classical Event
DOI: 10.1029/2024JA032986 Bibcode: 2024JGRA..12932986H

Henri, Pierre; Hajra, Rajkumar; Horne, Richard B. +8 more

The 23-24 April 2023 double-peak (SYM-H intensities of −179 and −233 nT) intense geomagnetic storm was caused by interplanetary magnetic field southward component Bs associated with an interplanetary fast-forward shock-preceded sheath (Bs of 25 nT), followed by a magnetic cloud (MC) (Bs of 33 nT), respectively. The…

2024 Journal of Geophysical Research (Space Physics)
Cluster 2
Kinematics and star formation of hub-filament systems in W49A
DOI: 10.1051/0004-6361/202348580 Bibcode: 2024A&A...688A..99Z

Li, Dalei; Tang, Xindi; Zhou, Jianjun +11 more


Aims: W49A is a prominent giant molecular cloud (GMC) that exhibits strong star formation activities, yet its structural and kinematic properties remain uncertain. Our study aims to investigate the large-scale structure and kinematics of W49A, and elucidate the role of filaments and hub-filament systems (HFSs) in its star formation activity. …

2024 Astronomy and Astrophysics
Herschel 2
Solar Energetic Proton Fluxes in Near-Earth Space on March 13-23, 2023
DOI: 10.1134/S0010952523600282 Bibcode: 2024CosRe..62..197V

Vlasova, N. A.; Bazilevskaya, G. A.; Ginzburg, E. A. +5 more

The results of studying the fluxes of solar protons with energies greater than 5 MeV in near-Earth space on March 13-23, 2023, are presented. The features of the period under study are no visible solar flare with which the beginning of the event could be associated and an untypical time profile of proton fluxes, as well as a long duration of the e…

2024 Cosmic Research
SOHO SolarOrbiter 2
Diffuse interstellar bands in the near-infrared: expanding the reddening range
DOI: 10.1093/mnras/stae1472 Bibcode: 2024MNRAS.532.2065C

Najarro, F.; Geballe, T. R.; Garcia, M. +2 more

We have investigated the behaviour of three strong near-infrared diffuse interstellar bands (DIBs) at λ13177 Å, λ14680 Å, and λ15272 Å, on a larger sample of sightlines and over a wider range of extinctions than previously studied, utilizing spectra from three observatories. We applied two telluric correction techniques to reduce atmospheric conta…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 2
Probing the strength of radial migration via churning by using metal-rich red giant stars from APOGEE
DOI: 10.1093/mnras/stae1736 Bibcode: 2024MNRAS.533..538L

Kordopatis, Georges; Feltzing, Sofia; Lehmann, Christian +1 more

Making use of the APOGEE DR17 catalogue with high quality data for 143 509 red giant branch stars we explore the strength of different mechanisms that causes a star to radially migrate in the Milky Way stellar disc. At any position in the disc we find stars that are more metal-rich than the local interstellar medium. This is surprising and normall…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 2
Production of s-process elements in asymptotic giant branch stars as revealed by Gaia/GSP-Spec abundances
DOI: 10.1051/0004-6361/202347188 Bibcode: 2024A&A...683A.138C

Recio-Blanco, A.; de Laverny, P.; Contursi, G. +2 more

Context. The recent parameterisation by the GSP-Spec module of Gaia/Radial Velocity Spectrometer stellar spectra has produced an homogeneous catalogue of about 174 000 asymptotic giant branch (AGB) stars. Among the 13 chemical elements presented in this Gaia third data release, the abundance of two of them (cerium and neodymium) have been estimate…

2024 Astronomy and Astrophysics
Gaia 2
The Massive and Distant Clusters of WISE Survey 2: A Stacking Analysis Investigating the Evolution of Star Formation Rates and Stellar Masses in Groups and Clusters
DOI: 10.3847/1538-4357/ad5545 Bibcode: 2024ApJ...972...27T

Alberts, Stacey; Connor, Thomas; Eisenhardt, Peter R. M. +8 more

The evolution of galaxies depends on their masses and local environments; understanding when and how environmental quenching starts to operate remains a challenge. Furthermore, studies of the high-redshift regime have been limited to massive cluster members, owing to sensitivity limits or small fields of view when the sensitivity is sufficient, in…

2024 The Astrophysical Journal
Herschel 2
Short-term variability of the transitional pulsar candidate CXOU J110926.4‑650224 from X-rays to infrared
DOI: 10.1051/0004-6361/202450915 Bibcode: 2024A&A...690A.220C

D'Avanzo, P.; Campana, S.; de Martino, D. +14 more

CXOU J110926.4‑650224 is a candidate transitional millisecond pulsar (tMSP) with X-ray and radio emission properties reminiscent of those observed in confirmed tMSPs in their X-ray 'subluminous' disc state. We present the results of observing campaigns that, for the first time, characterise the optical and near-infrared variability of this source …

2024 Astronomy and Astrophysics
Gaia XMM-Newton 2