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Systematic Study of AGN Clumpy Tori with Broadband X-Ray Spectroscopy: Updated Unified Picture of AGN Structure
DOI: 10.3847/1538-4357/abccce Bibcode: 2021ApJ...906...84O

Tanimoto, Atsushi; Ueda, Yoshihiro; Ogawa, Shoji +1 more

We present the results of a systematic, broadband X-ray spectral analysis of nearby active galactic nuclei (AGNs) with the X-ray clumpy torus model (XCLUMPY). By adding 16 AGNs newly analyzed in this paper, we study a total of 28 AGNs, including unabsorbed and absorbed AGNs taken from Ichikawa et al. and García-Bernete et al. This is the largest s…

2021 The Astrophysical Journal
XMM-Newton 40
Constraining primordial black holes as dark matter at JUNO
DOI: 10.1103/PhysRevD.103.043010 Bibcode: 2021PhRvD.103d3010W

Wang, Sai; Xia, Dong-Mei; Chang, Zhe +2 more

As an attractive candidate for dark matter, the primordial black holes (PBHs) in the mass range (8 ×1014∼1016) g could be detected via their Hawking radiation, including neutrinos and antineutrinos of three flavors. In this paper, we investigate the possibility to constrain the PBHs as dark matter by measuring (anti)neutrino …

2021 Physical Review D
INTEGRAL 40
All-sky visible and near infrared space astrometry
DOI: 10.1007/s10686-021-09705-z Bibcode: 2021ExA....51..783H

Tanga, Paolo; Ting, Yuan-Sen; Zwitter, Tomaž +27 more

The era of all-sky space astrometry began with the Hipparcos mission in 1989 and provided the first very accurate catalogue of apparent magnitudes, positions, parallaxes and proper motions of 120 000 bright stars at the milliarcsec (or milliarcsec per year) accuracy level. Hipparcos has now been superseded by the results of the Gaia mission. The s…

2021 Experimental Astronomy
Gaia Hipparcos 39
Comparing the pre-SNe feedback and environmental pressures for 6000 H II regions across 19 nearby spiral galaxies
DOI: 10.1093/mnras/stab2958 Bibcode: 2021MNRAS.508.5362B

Chevance, M.; Murphy, E. J.; Dale, D. A. +28 more

The feedback from young stars (i.e. pre-supernova) is thought to play a crucial role in molecular cloud destruction. In this paper, we assess the feedback mechanisms acting within a sample of 5810 H II regions identified from the PHANGS-MUSE survey of 19 nearby (<20 Mpc) star-forming, main-sequence spiral galaxies [log(M/M

2021 Monthly Notices of the Royal Astronomical Society
eHST 39
Multi-Annual Monitoring of the Water Vapor Vertical Distribution on Mars by SPICAM on Mars Express
DOI: 10.1029/2020JE006616 Bibcode: 2021JGRE..12606616F

Montmessin, Franck; Trokhimovskiy, Alexander; Bertaux, Jean-Loup +3 more

The distribution of water vapor with altitude has long remained a missing piece of the observational data set of water vapor on Mars. In this study, we present the first multi-annual survey of water vapor profile covering the altitude range from 0 to 100 km based on the SPICAM/Mars Express occultation measurements. During the aphelion season, wate…

2021 Journal of Geophysical Research (Planets)
MEx 39
Multiple Stellar Populations along the Red Horizontal Branch and Red Clump of Globular Clusters
DOI: 10.3847/1538-4357/abc882 Bibcode: 2021ApJ...906...76D

Milone, A. P.; Cordoni, G.; Marino, A. F. +5 more

We exploit multiband Hubble Space Telescope photometry to investigate multiple populations (MPs) along the red horizontal branches (HBs) and red clumps of 14 metal-rich globular clusters (GCs), including 12 Milky Way GCs and the Magellanic Cloud GCs NGC 1978 and NGC 416. Based on appropriate two-color diagrams, we find that the fraction of first-g…

2021 The Astrophysical Journal
Gaia eHST 39
Implementation of disequilibrium chemistry to spectral retrieval code ARCiS and application to 16 exoplanet transmission spectra. Indication of disequilibrium chemistry for HD 209458b and WASP-39b
DOI: 10.1051/0004-6361/202141548 Bibcode: 2021A&A...656A..90K

Min, Michiel; Kawashima, Yui

Context. The retrieval approach is currently a standard method for deriving atmospheric properties from observed spectra of exoplanets. However, the approach ignores disequilibrium chemistry in most current retrieval codes, which can lead to a misinterpretation of the metallicity or elemental abundance ratios of the atmosphere.
Aims: We have …

2021 Astronomy and Astrophysics
eHST 39
Physical properties of the ambient medium and of dense cores in the Perseus star-forming region derived from Herschel Gould Belt Survey observations
DOI: 10.1051/0004-6361/201936534 Bibcode: 2021A&A...645A..55P

André, Ph.; Arzoumanian, D.; Könyves, V. +20 more

The complex of star-forming regions in Perseus is one of the most studied due to its proximity (about 300 pc). In addition, its regions show variation in star-formation activity and age, with formation of low-mass and intermediate-mass stars. In this paper, we present analyses of images taken with the Herschel ESA satellite from 70 µm to 500…

2021 Astronomy and Astrophysics
Gaia Herschel 39
Compton-thick AGN in the NuSTAR Era VI: The Observed Compton-thick Fraction in the Local Universe
DOI: 10.3847/1538-4357/ac1c73 Bibcode: 2021ApJ...922..252T

Vignali, C.; Gilli, R.; Comastri, A. +11 more

We present the analysis of simultaneous Nuclear Spectroscopic Telescope Array (NuSTAR) and XMM-Newton data of eight Compton-thick active galactic nuclei (CT-AGN) candidates selected in the Swift-BAT 100 month catalog. This work is part of an ongoing effort to find and characterize all CT-AGN in the Local (z ≤ 0.05) Universe. We used two physically…

2021 The Astrophysical Journal
XMM-Newton 39
The Hawaii Infrared Parallax Program. V. New T-dwarf Members and Candidate Members of Nearby Young Moving Groups
DOI: 10.3847/1538-4357/abe3fa Bibcode: 2021ApJ...911....7Z

Siverd, Robert J.; Dupuy, Trent J.; Liu, Michael C. +2 more

We present a search for new planetary-mass members of nearby young moving groups (YMGs) using astrometry for 694 T and Y dwarfs, including 447 objects with parallaxes, mostly produced by recent large parallax programs from UKIRT and Spitzer. Using the BANYAN Σ and LACEwING algorithms, we identify 30 new candidate YMG members, with spectral types o…

2021 The Astrophysical Journal
Gaia 39