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Mid- and Far-infrared Color-Color Relations within Local Galaxies
DOI: 10.3847/1538-4357/ac558a Bibcode: 2022ApJ...928..120G

Calzetti, Daniela; Heyer, Mark; Gregg, Benjamin

We present an extensive archival analysis of a sample of local galaxies, combining multiwavelength data from GALEX, Spitzer, and Herschel to investigate "blue-side" mid-infrared (MIR) and "red-side" far-infrared (FIR) color-color correlations within the observed infrared spectral energy distributions. Our sample largely consists of the KINGFISH ga…

2022 The Astrophysical Journal
Herschel 8
Molecular and Atomic Clouds Associated with the Gamma-Ray Supernova Remnant Puppis A
DOI: 10.3847/1538-4357/ac90c6 Bibcode: 2022ApJ...938...94A

Rowell, G.; Fukui, Y.; Reynoso, E. M. +3 more

We have carried out a study of the interstellar medium (ISM) toward the shell-like supernova remnant (SNR) Puppis A using NANTEN CO and ATCA H I data. We synthesized a comprehensive picture of the SNR radiation by combining the ISM data with the gamma-ray and X-ray distributions. The ISM, both atomic and molecular gas, is dense and highly clumpy, …

2022 The Astrophysical Journal
XMM-Newton 8
High-resolution X-ray study of supernova remnant J0453.6-6829 with unusually high forbidden-to-resonance ratio
DOI: 10.1093/pasj/psac033 Bibcode: 2022PASJ...74..757K

Uchida, Hiroyuki; Tsuru, Takeshi Go; Tanaka, Takaaki +3 more

Recent high-resolution X-ray spectroscopy has revealed that several supernova remnants (SNRs) in the Large Magellanic Cloud (LMC) show unusually high forbidden-to-resonance (f/r) line ratios. While their origin is still uncertain and debated, most of these SNRs have asymmetric morphology and/or show evidence of interaction with dense material, whi…

2022 Publications of the Astronomical Society of Japan
XMM-Newton 8
The Gaia-ESO survey: A spectroscopic study of the young open cluster NGC 3293
DOI: 10.1051/0004-6361/202244112 Bibcode: 2022A&A...665A.108M

Gilmore, G.; Gosset, E.; Herrero, A. +24 more

We present a spectroscopic analysis of the GIRAFFE and UVES data collected by the Gaia-ESO survey for the young open cluster NGC 3293. Archive spectra from the same instruments obtained in the framework of the `VLT-FLAMES survey of massive stars' are also analysed. Atmospheric parameters, non-local thermodynamic equilibrium (LTE) chemical abundanc…

2022 Astronomy and Astrophysics
Gaia 8
Hubble Space Telescope Observations of Active Asteroid P/2020 O1 (Lemmon-PANSTARRS)
DOI: 10.3847/2041-8213/ac78de Bibcode: 2022ApJ...933L..15K

Mutchler, Max; Jewitt, David; Agarwal, Jessica +3 more

We present Hubble Space Telescope observations of active asteroid P/2020 O1 taken to examine its development for a year after perihelion. We find that the mass loss peaks at ≲1 kg s-1 in 2020 August and then declines to nearly zero over four months. Long-duration mass loss (~180 days) is consistent with a sublimation origin, indicating …

2022 The Astrophysical Journal
eHST 8
Albedo variegation on Comet 67P/Churyumov-Gerasimenko
DOI: 10.1093/mnras/stac2456 Bibcode: 2022MNRAS.516.5125D

Buratti, Bonnie J.; Hicks, Michael D.; Davidsson, Björn J. R.

We here study the level of albedo variegation on the nucleus of Comet 67P/Churyumov-Gerasimenko. This is done by fitting the parameters of a standard photometric phase function model to disc-average radiance factor data in images acquired by the Rosetta/OSIRIS Narrow Angle Camera in the orange filter. Local discrepancies between the observed radia…

2022 Monthly Notices of the Royal Astronomical Society
Rosetta 8
Impact of bar resonances in the velocity-space distribution of the solar neighbourhood stars in a self-consistent N-body Galactic disc simulation
DOI: 10.1093/mnras/stac1379 Bibcode: 2022MNRAS.514..460A

Fujii, Michiko S.; Portegies Zwart, Simon; Baba, Junichi +3 more

The velocity-space distribution of the solar neighbourhood stars shows complex substructures. Most of the previous studies use static potentials to investigate their origins. Instead we use a self-consistent N-body model of the Milky Way, whose potential is asymmetric and evolves with time. In this paper, we quantitatively evaluate the similaritie…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 8
An X-ray fading, UV brightening QSO at z ≈ 6
DOI: 10.1051/0004-6361/202243403 Bibcode: 2022A&A...663A.159V

Bauer, F. E.; Brandt, W. N.; Vignali, C. +13 more

Explaining the existence of super massive black holes (SMBHs) with MBH ≳ 108 M at z ≳ 6 is a persistent challenge to modern astrophysics. Multiwavelength observations of z ≳ 6 quasi-stellar objects (QSOs) reveal that, on average, their accretion physics is similar to that of their counterparts at lower redshift. H…

2022 Astronomy and Astrophysics
XMM-Newton 8
Redshift space three-point correlation function of IGM at z < 0.48
DOI: 10.1093/mnras/stab3308 Bibcode: 2022MNRAS.509.4585M

Srianand, Raghunathan; Gaikwad, Prakash; Maitra, Soumak +1 more

Ly α forest decomposed into Voigt profile components allows us to study clustering properties of the intergalactic-medium and its dependence on various physical quantities. Here, we report the first detections of probability excess of low-z (i.e z < 0.48) Ly α absorber triplets over redshift-space scale of r ≤ 8 pMpc (Mpc in physica…

2022 Monthly Notices of the Royal Astronomical Society
eHST 8
An old warm Jupiter orbiting the metal-poor G-dwarf TOI-5542
DOI: 10.1051/0004-6361/202244077 Bibcode: 2022A&A...668A..29G

Jordán, Andrés; Stassun, Keivan G.; Worters, Hannah L. +30 more

We report the discovery of a 1.32−0.10+0.10 MJup planet orbiting on a 75.12 day period around the G3V 10.8−3.6+2.1 Gyr old star TOI-5542 (TIC 466206508; TYC 9086-1210-1). The planet was first detected by the Transiting Exoplanet Survey Satellite (TESS) as a single transit event in TESS Sector …

2022 Astronomy and Astrophysics
Gaia 7