Search Publications

AGNs in post-mergers from the ultraviolet near infrared optical northern survey
DOI: 10.1093/mnras/stad088 Bibcode: 2023MNRAS.519.6149B

Ellison, Sara L.; Bickley, Robert W.; Patton, David R. +1 more

The kinematic disturbances associated with major galaxy mergers are known to produce gas inflows, which in turn may trigger accretion onto the supermassive black holes (SMBH) of the participant galaxies. While this effect has been studied in galaxy pairs, the frequency of active galactic nuclei (AGNs) in fully coalesced post-merger systems is poor…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 21
The Cosmic Ultraviolet Baryon Survey: Empirical Characterization of Turbulence in the Cool Circumgalactic Medium
DOI: 10.3847/2041-8213/acf85b Bibcode: 2023ApJ...955L..25C

Faucher-Giguère, Claude-André; Johnson, Sean D.; Zahedy, Fakhri S. +11 more

This paper reports the first measurement of the relationship between turbulent velocity and cloud size in the diffuse circumgalactic medium (CGM) in typical galaxy halos at redshift z ≈ 0.4-1. Through spectrally resolved absorption profiles of a suite of ionic transitions paired with careful ionization analyses of individual components, cool clump…

2023 The Astrophysical Journal
eHST 21
Measuring the Dust Masses of Protoplanetary Disks in Lupus with ALMA: Evidence That Disks Can Be Optically Thick at 3 mm
DOI: 10.3847/1538-4357/aca52b Bibcode: 2023ApJ...942....4X

Ribas, Á.; Macías, E.; Espaillat, C. C. +2 more

Accurate disk mass measurements are necessary to constrain disk evolution and the timescale of planet formation, but such measurements are difficult to make and are very dependent on assumptions. Here, we look at the assumption that the disk is optically thin at radio wavelengths and the effect of this assumption on measurements of disk dust mass.…

2023 The Astrophysical Journal
Gaia Herschel 21
Bright extragalactic ALMA redshift survey (BEARS) III: detailed study of emission lines from 71 Herschel targets
DOI: 10.1093/mnras/stad784 Bibcode: 2023MNRAS.521.5508H

Berta, S.; Ivison, R. J.; Omont, A. +55 more

We analyse the molecular and atomic emission lines of 71 bright Herschel-selected galaxies between redshifts 1.4 and 4.6 detected by the Atacama Large Millimeter/submillimeter Array. These lines include a total of 156 CO, [C I], and H2O emission lines. For 46 galaxies, we detect two transitions of CO lines, and for these galaxies we fin…

2023 Monthly Notices of the Royal Astronomical Society
Herschel 21
Hunting for C-rich long-period variable stars in the Milky Way's bar-bulge using unsupervised classification of Gaia BP/RP spectra
DOI: 10.1093/mnras/stad574 Bibcode: 2023MNRAS.521.2745S

Matsunaga, Noriyuki; Sanders, Jason L.

The separation of oxygen- and carbon-rich asymptotic giant branch sources is crucial for their accurate use as local and cosmological distance and age/metallicity indicators. We investigate the use of unsupervised learning algorithms for classifying the chemistry of long-period variables from Gaia DR3's BP/RP spectra. Even in the presence of signi…

2023 Monthly Notices of the Royal Astronomical Society
AKARI Gaia 21
First Evidence of Multi-iron Subpopulations in the Bulge Fossil Fragment Candidate Liller 1
DOI: 10.3847/1538-4357/acd382 Bibcode: 2023ApJ...951...17C

Cadelano, Mario; Pallanca, Cristina; Dalessandro, Emanuele +9 more

In the context of a project aimed at characterizing the properties of the so-called Bulge Fossil Fragments (the fossil remnants of the bulge formation epoch), here we present the first determination of the metallicity distribution of Liller 1. For a sample of 64 individual member stars we used ESO-MUSE spectra to measure the equivalent width of th…

2023 The Astrophysical Journal
eHST 21
Multiple injections of energetic electrons associated with the flare and CME event on 9 October 2021
DOI: 10.1051/0004-6361/202245716 Bibcode: 2023A&A...675A..27J

Vainio, R.; Wiegelmann, T.; Krupar, V. +12 more

Context. We study the solar energetic particle (SEP) event observed on 9 October 2021 by multiple spacecraft, including Solar Orbiter. The event was associated with an M1.6 flare, a coronal mass ejection, and a shock wave. During the event, high-energy protons and electrons were recorded by multiple instruments located within a narrow longitudinal…

2023 Astronomy and Astrophysics
SOHO SolarOrbiter 21
A NOEMA Molecular Line Scan of the Hubble Deep Field North: Improved Constraints on the CO Luminosity Functions and Cosmic Density of Molecular Gas
DOI: 10.3847/1538-4357/acb4f0 Bibcode: 2023ApJ...945..111B

Carilli, Chris; Boogaard, Leindert A.; Pety, Jérôme +9 more

We present measurements of the CO luminosity functions (LFs) and the evolution of the cosmic molecular gas density out to z ~ 6 based on an 8.5 arcmin2 spectral scan survey at 3 mm of the iconic Hubble Deep Field North (HDF-N) observed with the NOrthern Extended Millimeter Array (NOEMA). We use matched filtering to search for line emiss…

2023 The Astrophysical Journal
Herschel eHST 21
Kinematic analysis of the Large Magellanic Cloud using Gaia DR3
DOI: 10.1051/0004-6361/202244601 Bibcode: 2023A&A...669A..91J

Luri, X.; Masana, E.; Antoja, T. +6 more

Context. The high quality of the Gaia mission data has allowed for studies of the internal kinematics of the Large Magellanic Cloud (LMC) to be undertaken in unprecedented detail, providing insights into the non-axisymmetric structure of its disc. Recent works by the Gaia Collaboration have already made use of the excellent proper motions of Gaia …

2023 Astronomy and Astrophysics
Gaia 21
Astrophysical properties of 15062 Gaia DR3 gravity-mode pulsators. Pulsation amplitudes, rotation, and spectral line broadening
DOI: 10.1051/0004-6361/202245713 Bibcode: 2023A&A...672A.183A

De Ridder, J.; Aerts, C.; Molenberghs, G.

Context. Gravito-inertial asteroseismology came into existence thanks to high-precision CoRoT and Kepler space photometric light curves. So far, it has given rise to the internal rotation frequency of a few hundred intermediate-mass stars, yet only several tens of these have been weighed, sized, and age-dated with high precision using asteroseismi…

2023 Astronomy and Astrophysics
Gaia 21