Search Publications

AGN Selection and Demographics in GOODS-S/HUDF from X-Ray to Radio
DOI: 10.3847/1538-4357/ac9e5d Bibcode: 2022ApJ...941..191L

Lyu, Jianwei; Rieke, George H.; Alberts, Stacey +1 more

We present a comprehensive census of the active galactic nuclei (AGNs) in the GOODS-S/HUDF region from the X-ray to the radio, covering both the obscured and unobscured populations. This work includes a robust analysis of the source optical to mid-IR spectral energy distributions (SEDs) featuring (semi)empirical AGN and galaxy dust emission models…

2022 The Astrophysical Journal
AKARI eHST 57
GOALS-JWST: Tracing AGN Feedback on the Star-forming Interstellar Medium in NGC 7469
DOI: 10.3847/2041-8213/ac9ebf Bibcode: 2022ApJ...941L..36L

Inami, Hanae; Böker, Torsten; Law, David R. +34 more

We present James Webb Space Telescope (JWST) Mid-Infrared Instrument (MIRI) integral-field spectroscopy of the nearby merging, luminous infrared galaxy, NGC 7469. This galaxy hosts a Seyfert type-1.5 nucleus, a highly ionized outflow, and a bright, circumnuclear star-forming ring, making it an ideal target to study active galactic nucleus (AGN) fe…

2022 The Astrophysical Journal
AKARI JWST 51
Asteroid taxonomy from cluster analysis of spectrometry and albedo
DOI: 10.1051/0004-6361/202243587 Bibcode: 2022A&A...665A..26M

Carry, B.; Mahlke, M.; Mattei, P. -A.

Context. The classification of the minor bodies of the Solar System based on observables has been continuously developed and iterated over the past 40 yr. While prior iterations followed either the availability of large observational campaigns or new instrumental capabilities opening new observational dimensions, we see the opportunity to improve …

2022 Astronomy and Astrophysics
AKARI 50
Planet populations inferred from debris discs. Insights from 178 debris systems in the ISPY, LEECH, and LIStEN planet-hunting surveys
DOI: 10.1051/0004-6361/202142720 Bibcode: 2022A&A...659A.135P

Gennaro, Mario; Launhardt, Ralf; Kennedy, Grant M. +11 more

We know little about the outermost exoplanets in planetary systems because our detection methods are insensitive to moderate-mass planets on wide orbits. However, debris discs can probe the outer-planet population because dynamical modelling of observed discs can reveal properties of perturbing planets. We use four sculpting and stirring arguments…

2022 Astronomy and Astrophysics
AKARI Gaia 42
Polycyclic aromatic hydrocarbons in Seyfert and star-forming galaxies
DOI: 10.1093/mnras/stab3127 Bibcode: 2022MNRAS.509.4256G

Rigopoulou, D.; Pereira-Santaella, M.; Alonso-Herrero, A. +3 more

Polycyclic Aromatic Hydrocarbons (PAHs) are carbon-based molecules resulting from the union of aromatic rings and related species, which are likely responsible for strong infrared emission features. In this work, using a sample of 50 Seyfert galaxies (DL < 100 Mpc) we compare the circumnuclear (inner kpc) PAH emission of AGN to that …

2022 Monthly Notices of the Royal Astronomical Society
AKARI ISO 39
BASS XXXII: Studying the Nuclear Millimeter-wave Continuum Emission of AGNs with ALMA at Scales ≲100-200 pc
DOI: 10.3847/1538-4357/ac8794 Bibcode: 2022ApJ...938...87K

Baba, Shunsuke; Imanishi, Masatoshi; Ueda, Yoshihiro +25 more

To understand the origin of nuclear (≲100 pc) millimeter-wave (mm-wave) continuum emission in active galactic nuclei (AGNs), we systematically analyzed subarcsecond resolution Band-6 (211-275 GHz) Atacama Large Millimeter/submillimeter Array data of 98 nearby AGNs (z < 0.05) from the 70 month Swift/BAT catalog. The sample, almost unbiased for o…

2022 The Astrophysical Journal
AKARI Herschel 37
A Survey of CO, CO2, and H2O in Comets and Centaurs
DOI: 10.3847/PSJ/ac960d Bibcode: 2022PSJ.....3..247H

Bauer, James; Harrington Pinto, Olga; Womack, Maria +1 more

CO and CO2 are the two dominant carbon-bearing molecules in comae and have major roles in driving activity. Their relative abundances also provide strong observational constraints to models of solar system formation and evolution but have never been studied together in a large sample of comets. We carefully compiled and analyzed publish…

2022 The Planetary Science Journal
AKARI ISO 32
The Debiased Compositional Distribution of MITHNEOS: Global Match between the Near-Earth and Main-belt Asteroid Populations, and Excess of D-type Near-Earth Objects
DOI: 10.3847/1538-3881/ac532f Bibcode: 2022AJ....163..165M

Granvik, Mikael; Carry, Benoit; Marsset, Michaël +10 more

We report 491 new near-infrared spectroscopic measurements of 420 near-Earth objects (NEOs) collected on the NASA InfraRed Telescope Facility as part of the MIT-Hawaii NEO Spectroscopic Survey. These measurements were combined with previously published data from Binzel et al. and bias-corrected to derive the intrinsic compositional distribution of…

2022 The Astronomical Journal
AKARI 29
Mira variables in the Milky Way's nuclear stellar disc: discovery and classification
DOI: 10.1093/mnras/stac2274 Bibcode: 2022MNRAS.517..257S

Smith, Leigh C.; Matsunaga, Noriyuki; Minniti, Dante +3 more

The properties of the Milky Way's nuclear stellar disc give crucial information on the epoch of bar formation. Mira variables are promising bright candidates to study the nuclear stellar disc, and through their period-age relation dissect its star formation history. We report on a sample of 1782 Mira variable candidates across the central $3\times…

2022 Monthly Notices of the Royal Astronomical Society
AKARI Gaia Herschel 27
Upper mass-loss limits and clumping in the intermediate and outer wind regions of OB stars
DOI: 10.1051/0004-6361/202040116 Bibcode: 2022A&A...658A..61R

Puls, J.; Najarro, F.; Traficante, A. +4 more

Context. Mass loss is a key parameter throughout the evolution of massive stars, and it determines the feedback with the surrounding interstellar medium. The presence of inhomogeinities in stellar winds (clumping) leads to severe discrepancies not only among different mass-loss rate diagnostics, but also between empirical estimates and theoretical…

2022 Astronomy and Astrophysics
AKARI Gaia Herschel 27