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The properties of the X-ray corona in the distant (z = 3.91) quasar APM 08279+5255
DOI: 10.1051/0004-6361/202142642 Bibcode: 2022A&A...662A..98B

Cappi, M.; Vignali, C.; Gilli, R. +7 more

We present new joint XMM-Newton and NuSTAR observations of APM 08279+5255, a gravitationally-lensed, broad-absorption line quasar (z = 3.91). After showing a fairly stable flux (f2 − 10 ≃ 4 − 5.5 × 10−13 erg s−1) from 2000 to 2008, APM 08279+5255 was found in a fainter state in the latest X-ray exposures (f2 −…

2022 Astronomy and Astrophysics
XMM-Newton 11
Identification of three cataclysmic variables detected by the ART-XC and eROSITA telescopes on board the SRG during the all-sky X-ray survey
DOI: 10.1051/0004-6361/202141777 Bibcode: 2022A&A...661A..39Z

Sunyaev, R.; Sazonov, S.; Burenin, R. +6 more

We report the discovery of three cataclysmic variables in the data of the first year of the all-sky X-ray survey by the SRG orbital observatory. The sources were selected for their brightness in the 4-12 keV band in the data of the Mikhail Pavlinsky ART-XC telescope. They are also detected by the eROSITA telescope, which provides accurate localiza…

2022 Astronomy and Astrophysics
Gaia 11
Dual storage and release of molecular oxygen in comet 67P/Churyumov-Gerasimenko
DOI: 10.1038/s41550-022-01614-1 Bibcode: 2022NatAs...6..724L

Mousis, Olivier; Trattner, Karlheinz J.; Lunine, Jonathan I. +7 more

One of the biggest surprises of the Rosetta mission was the detection of O2 in the coma of 67P/Churyumov-Gerasimenko in remarkably high abundances. The measured levels of O2 in the coma are generally assumed to reflect the overall abundance and chemical origin of cometary O2 in the nucleus. Along with its strong as…

2022 Nature Astronomy
Rosetta 11
Characterization of Kepler targets based on medium-resolution LAMOST spectra analyzed with ROTFIT
DOI: 10.1051/0004-6361/202243268 Bibcode: 2022A&A...664A..78F

De Cat, P.; Frasca, A.; Wang, J. X. +7 more


Aims: In this work we present the results of our analysis of 16 300 medium-resolution LAMOST spectra of late-type stars in the Kepler field with the aim of determining the stellar parameters, activity level, lithium atmospheric content, and binarity.
Methods: We have used a version of the code ROTFIT specifically developed for the LAMOST…

2022 Astronomy and Astrophysics
AKARI Gaia 11
The LHS 1678 System: Two Earth-sized Transiting Planets and an Astrometric Companion Orbiting an M Dwarf Near the Convective Boundary at 20 pc
DOI: 10.3847/1538-3881/ac32e3 Bibcode: 2022AJ....163..151S

Kostov, Veselin B.; Torres, Guillermo; Barclay, Thomas +48 more

We present the Transiting Exoplanet Survey Satellite (TESS) discovery of the LHS 1678 (TOI-696) exoplanet system, comprised of two approximately Earth-sized transiting planets and a likely astrometric brown dwarf orbiting a bright (V J = 12.5, K s = 8.3) M2 dwarf at 19.9 pc. The two TESS-detected planets are of radius 0.7…

2022 The Astronomical Journal
Gaia 11
Massive Black Hole Formation in Dense Stellar Environments: Enhanced X-Ray Detection Rates in High-velocity Dispersion Nuclear Star Clusters
DOI: 10.3847/1538-4357/ac5f51 Bibcode: 2022ApJ...929...84B

Stone, Nicholas C.; Ostriker, Jeremiah P.; Baldassare, Vivienne F. +2 more

We analyze Chandra X-ray Observatory imaging of 108 galaxies hosting nuclear star clusters (NSCs) to search for signatures of massive black holes (BHs). NSCs are extremely dense stellar environments with conditions that can theoretically facilitate massive BH formation. Recent work by Stone et al. finds that sufficiently dense NSCs should be unsta…

2022 The Astrophysical Journal
eHST 11
High-resolution ALMA observations of V4046 Sgr: a circumbinary disc with a thin ring
DOI: 10.1093/mnras/stab3440 Bibcode: 2022MNRAS.510.1248M

Garufi, Antonio; Pérez, Sebastián; Casassus, Simon +8 more

The nearby V4046 Sgr spectroscopic binary hosts a gas-rich disc known for its wide cavity and dusty ring. We present high resolution (~20 mas or 1.4 au) ALMA observations of the 1.3 mm continuum of V4046 Sgr which, combined with SPHERE-IRDIS polarised images and a well-sampled spectral energy distribution (SED), allow us to propose a physical mode…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 11
On the dynamical evolution of Cepheids in star clusters
DOI: 10.1051/0004-6361/202142134 Bibcode: 2022A&A...659A.169D

Anderson, Richard I.; Kroupa, Pavel; Dinnbier, František

We investigated the occurrence of classical (type-I) Cepheid variable stars (henceforth Cepheids) in dynamically evolving star clusters from birth to an age of approximately 300 Myr. The clusters are modelled by the Aarseth code NBODY6, and they feature a realistic stellar initial mass function and initial binary star population, single star and b…

2022 Astronomy and Astrophysics
Gaia 11
Investigating the Low-flux States in Six Intermediate Polars
DOI: 10.3847/1538-4357/ac5682 Bibcode: 2022ApJ...928..164C

Littlefield, Colin; Heinke, Craig O.; Mukai, Koji +30 more

We present optical photometry of six intermediate polars that exhibit transitions to a low-flux state. For four of these systems, DW Cnc, V515 And, V1223 Sgr, and RX J2133.7+5107, we are able to perform timing analysis in and out of the low states. We find that, for DW Cnc and V515 And, the dominant periodicities in the light curves change as the …

2022 The Astrophysical Journal
Gaia 11
A systematic comparison of galaxy cluster temperatures measured with NuSTAR and Chandra
DOI: 10.1093/mnras/stac3055 Bibcode: 2022MNRAS.517.5594W

Wik, D. R.; Gastaldello, F.; Maughan, B. J. +2 more

Temperature measurements of galaxy clusters are used to determine their masses, which in turn are used to determine cosmological parameters. However, systematic differences between the temperatures measured by different telescopes imply a significant source of systematic uncertainty on such mass estimates. We perform the first systematic compariso…

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 11