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X-Ray and Near-Infrared Observations of the Middle-aged Pulsar B1055-52, Its Multiwavelength Spectrum, and Proper Motion
DOI: 10.3847/1538-4357/acd9d1 Bibcode: 2023ApJ...952..134P

Pavlov, G. G.; Kargaltsev, O.; Hare, J. +1 more

Previous observations of the middle-aged γ-ray, X-ray, and radio pulsar B1055-52 indicated some peculiarities, such as a suspected changing of the X-ray flux and spectral parameters, a large excess of the alleged thermal component of the UV spectrum over the Rayleigh-Jeans extension of the X-ray thermal spectrum, and a possible double break in the…

2023 The Astrophysical Journal
Gaia XMM-Newton eHST 4
Exploring the short-term variability of H α and H β emissions in a sample of M dwarfs
DOI: 10.1093/mnras/stad2222 Bibcode: 2023MNRAS.524.6085K

Queiroz, A. B. A.; Fernández-Trincado, José G.; Kumar, Vipin +2 more

The time-scales of variability in active M dwarfs can be related to their various physical parameters. Thus, it is important to understand such variability to decipher the physics of these objects. In this study, we have performed the low resolution (~5.7 Å) spectroscopic monitoring of 83 M dwarfs (M0-M6.5) to study the variability of H α/H β emis…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 4
DeGaPe 35: Amateur discovery of a new southern symbiotic star
DOI: 10.1016/j.newast.2022.101943 Bibcode: 2023NewA...9801943P

Charbonnel, Stéphane; Garde, Olivier; Merc, Jaroslav +6 more

In this work, we present the discovery and characterization of a new southern S-type symbiotic star, DeGaPe 35. We have obtained the low-resolution spectroscopic observations and supplemented them with the photometry from Gaia DR3 and other surveys. The optical spectra of this target show prominent emission lines, including highly ionized [Fe VII]…

2023 New Astronomy
Gaia 4
Detection of Multiple Phase Space Overdensities of GSE Stars by Orbit Integration
DOI: 10.3847/1538-4357/acd33a Bibcode: 2023ApJ...950..151W

Zhao, Gang; Chen, Yuqin; Li, Chengdong +5 more

In N-body simulations, nearly radial mergers can form shell-like overdensities in the sky position and phase space (r - v r ) due to the combination of dynamical friction and tidal stripping. The merger event of Gaia-Sausage-Enceladus (GSE) has provided a unique opportunity to study the shells in the phase space. To search for them, we…

2023 The Astrophysical Journal
Gaia 4
The spectra of IceCube Neutrino (SIN) candidate sources - IV. Spectral energy distributions and multiwavelength variability
DOI: 10.1093/mnras/stad2724 Bibcode: 2023MNRAS.526..661K

Giommi, Paolo; Padovani, Paolo; Karl, Martina

We present hybrid spectral energy distributions, combining photon, and neutrino fluxes, for a sample of blazars, which are candidate IceCube neutrino sources. We furthermore check for differences in our sources' variability in the near-infrared, optical, X-ray, and γ-ray bands compared to a sample of non-neutrino source candidate blazars, and inve…

2023 Monthly Notices of the Royal Astronomical Society
Exosat XMM-Newton 4
Salt Constructs in Paleo-Lake Basins as High-Priority Astrobiology Targets
DOI: 10.3390/rs15020314 Bibcode: 2023RemS...15..314P

Cabrol, Nathalie A.; Phillips, Michael S.; McInenly, Michael +4 more

In extreme environments, microbial organisms reside in pockets with locally habitable conditions. Micro-climates conducive to the persistence of life in an otherwise inhospitable environment—"refugia"—are spatially restricted and can be micro- to centimeters in extent. If martian microbes are preserved in fossil refugia, this presents a double-edg…

2023 Remote Sensing
MEx 4
The Isaac Newton Telescope Monitoring Survey of Local Group Dwarf Galaxies. V. The Star Formation History of Sagittarius Dwarf Irregular Galaxy Derived from Long-period Variable Stars
DOI: 10.3847/1538-4357/aca471 Bibcode: 2023ApJ...942...33P

Javadi, Atefeh; Saremi, Elham; van Loon, Jacco Th. +7 more

We conducted an optical monitoring survey of the Sagittarius dwarf irregular galaxy (SagDIG) during the period of 2016 June-2017 October, using the 2.5 m Isaac Newton Telescopeat La Palama. Our goal was to identify long-period variable stars (LPVs), namely, asymptotic giant branch stars (AGBs) and red supergiant stars, to obtain the star formation…

2023 The Astrophysical Journal
Gaia 4
Statistical Study of Release Time and Its Energy Dependence of In Situ Energetic Electrons in Impulsive Solar Flares
DOI: 10.1029/2022JA030939 Bibcode: 2023JGRA..12830939W

Li, Gang; Wang, Linghua; Zhao, Lulu +3 more

Using the fraction velocity dispersion analysis method, it has been shown recently that in two impulsive solar energetic electron (SEE) events, the release times of near-relativistic electrons at the Sun for outward-propagating electrons are energy dependent and are delayed compared to those of the downward-propagating electrons. In this work, we …

2023 Journal of Geophysical Research (Space Physics)
SOHO 4
Steadiness of Coronal Heating
DOI: 10.3847/1538-4357/acf83a Bibcode: 2023ApJ...957...25J

Judge, P. G.

The EUI instrument on the Solar Orbiter spacecraft has obtained the most stable, high-resolution images of the solar corona from its orbit with a perihelion near 0.4 au. A sequence of 360 images obtained at 17.1 nm, between 2022 October 25 19:00 and 19:30 UT, is scrutinized. One image pixel corresponds to 148 km at the solar surface. The widely he…

2023 The Astrophysical Journal
SolarOrbiter 4
Universal Upper End of the Stellar Initial Mass Function in the Young and Compact LEGUS Clusters
DOI: 10.3847/1538-4357/aceb5c Bibcode: 2023ApJ...954..136J

Schaerer, Daniel; Smith, Linda J.; Calzetti, Daniela +21 more

We investigate the variation in the upper end of the stellar initial mass function (uIMF) in 375 young and compact star clusters in five nearby galaxies within ~5 Mpc. All the young stellar clusters (YSCs) in the sample have ages ≲ 4 Myr and masses above 500 M , according to standard stellar models. The YSC catalogs were produced from …

2023 The Astrophysical Journal
eHST 4