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The globular cluster system of the nearest Seyfert II galaxy Circinus
DOI: 10.1051/0004-6361/202243154 Bibcode: 2023A&A...670A..18O

Minniti, D.; Alonso-García, J.; Gómez, M. +7 more

Context. The globular cluster (GC) system of Circinus galaxy has not been probed previously partly because of the location of the galaxy at −3.8° Galactic latitude, which suffers severely from interstellar extinction, stellar crowding, and Galactic foreground contamination. However, the deep near-infrared (NIR) photometry by the VISTA Variables in…

2023 Astronomy and Astrophysics
Gaia 5
Harnessing the Hubble Space Telescope Archives: A Catalog of 21,926 Interacting Galaxies
DOI: 10.3847/1538-4357/acc0ff Bibcode: 2023ApJ...948...40O

Mantha, Kameswara Bharadwaj; Simmons, Brooke D.; Merín, Bruno +13 more

Mergers play a complex role in galaxy formation and evolution. Continuing to improve our understanding of these systems requires ever larger samples, which can be difficult (even impossible) to select from individual surveys. We use the new platform ESA Datalabs to assemble a catalog of interacting galaxies from the Hubble Space Telescope science …

2023 The Astrophysical Journal
XMM-Newton eHST 5
XTE J1906+090: a persistent low-luminosity Be X-ray binary
DOI: 10.1093/mnras/stad1494 Bibcode: 2023MNRAS.523.1192S

Sidoli, L.; La Palombara, N.; Bird, A. J. +1 more

We present new results from INTEGRAL and Swift observations of the hitherto poorly studied and unidentified X-ray source XTE J1906+090. A bright hard X-ray outburst (luminosity of ~1036 erg s-1 above 20 keV) has been discovered with INTEGRAL observations in 2010, this being the fourth outburst ever detected from the source. S…

2023 Monthly Notices of the Royal Astronomical Society
Gaia INTEGRAL XMM-Newton 5
The MUSE Ultra Deep Field (MUDF). IV. A pair of X-ray weak quasars at the heart of two extended Lyα nebulae
DOI: 10.1093/mnras/stad2564 Bibcode: 2023MNRAS.525.4388L

Haardt, Francesco; Rafelski, Marc; Lusso, Elisabeta +10 more

We present the results obtained from follow-up observations of the MUSE Ultra Deep Field (MUDF) at X-ray energies with XMM-Newton. The MUDF is centred on a unique field with two bright, physically associated quasars at z ≃ 3.23, separated by ~500 kpc in projection. Both quasars are embedded within extended Lyα nebulae (${\gtrsim}100\,{\rm kpc}$ at…

2023 Monthly Notices of the Royal Astronomical Society
XMM-Newton eHST 5
Long-Lived and Continual Volcanic Eruptions, Tectonic Activity, Pit Chains Formation, and Boulder Avalanches in Northern Tharsis Region: Implications for Late Amazonian Geodynamics and Seismo-Tectonic Processes on Mars
DOI: 10.1029/2022JE007511 Bibcode: 2023JGRE..12807511K

Kumar, P. Senthil; Krishnan, Vivek

Tharsis is the largest volcanic province on Mars. It consists of a few large shield volcanoes, one of which is Alba Mons (AM), located in northern Tharsis, with the Ceraunius Fossae (CF) graben system to the south of it. Previous workers argued in favor of episodic building of Tharsis volcanoes. In contrast, we show that volcanism in the AM and CF…

2023 Journal of Geophysical Research (Planets)
MEx 5
Morphology of Star-forming Clumps in Ram-pressure Stripped Galaxies as Seen by HST
DOI: 10.3847/1538-4357/acfed6 Bibcode: 2023ApJ...958...73G

Scarlata, Claudia; Calzetti, Daniela; Vulcani, Benedetta +9 more

We characterize the morphological properties of a statistically relevant sample of Hα and UV young star-forming clumps and optical complexes, observed with the Hubble Space Telescope in six galaxies of the GASP sample undergoing ram pressure stripping. The catalogs comprise 2406 (323 in the tails) Hα clumps, 3750 (899) UV clumps, and 424 tail opti…

2023 The Astrophysical Journal
eHST 5
The spectroscopic orbit of HD 168112 A,B in NGC 6604: another massive binary target for interferometry
DOI: 10.1093/mnras/stad2657 Bibcode: 2023MNRAS.525.6084P

Simón-Díaz, S.; Gamen, R.; Maíz Apellániz, J. +8 more

We present the first spectroscopic orbit of the O-type double-lined star HD 168112 A,B. We analyse 101 high-resolution optical spectra identifying the absorption lines of both components. The orbital solution presents a relatively long period, P = 513.52 ± 0.01 d, and a high eccentricity, e = 0.743 ± 0.005. The binary system consists of two very s…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 5
Dynamics and clouds in planetary atmospheres from telescopic observations
DOI: 10.1007/s00159-023-00150-9 Bibcode: 2023A&ARv..31....5S

Sánchez-Lavega, Agustín; Irwin, Patrick; García Muñoz, Antonio

This review presents an insight into our current knowledge of the atmospheres of the planets Venus, Mars, Jupiter, Saturn, Uranus and Neptune, the satellite Titan, and those of exoplanets. It deals with the thermal structure, aerosol properties (hazes and clouds, dust in the case of Mars), chemical composition, global winds, and selected dynamical…

2023 Astronomy and Astrophysics Review
eHST JWST 5
The first X-ray look at SMSS J114447.77-430859.3: the most luminous quasar in the last 9 Gyr
DOI: 10.1093/mnras/stad952 Bibcode: 2023MNRAS.522.5217K

Salvato, M.; Buchner, J.; Nandra, K. +18 more

SMSS J114447.77-430859.3 (z = 0.83) has been identified in the SkyMapper Southern Survey as the most luminous quasar in the last $\sim 9\, \rm Gyr$ . In this paper, we report on the eROSITA/Spectrum-Roentgen-Gamma (SRG) observations of the source from the eROSITA All Sky Survey, along with presenting results from recent monitoring performed using …

2023 Monthly Notices of the Royal Astronomical Society
XMM-Newton 5
HH 80/81: Structure and Kinematics of the Fastest Protostellar Outflow
DOI: 10.3847/1538-4357/acf028 Bibcode: 2023ApJ...958...99B

Bally, John; Reipurth, Bo

Hubble Space Telescope (HST) images obtained in 2018 are combined with archival HST data taken in 1995 to detect changes and measure proper motions in the HH 80/81 shock complex, which is powered by the fastest known jet driven by a forming star, the massive object IRAS 18162-2048. Some persistent features close to the radio jet axis have proper m…

2023 The Astrophysical Journal
eHST 5