Search Publications

Halo densities and pericenter distances of the bright Milky Way satellites as a test of dark matter physics
DOI: 10.1093/mnras/stae1716 Bibcode: 2024MNRAS.532.4157A

Andrade, Kevin E.; Kaplinghat, Manoj; Valli, Mauro

We provide new constraints on the dark matter halo density profile of Milky Way (MW) dwarf spheroidal galaxies (dSphs) using the phase-space distribution function (DF) method. After assessing the systematics of the approach against mock data from the Gaia Challenge project, we apply the DF analysis to the entire kinematic sample of well-measured M…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 5
Transit spectroscopy of K2-33b with subaru/IRD: Spin-Orbit alignment and tentative atmospheric helium
DOI: 10.1093/mnras/stae998 Bibcode: 2024MNRAS.530.3117H

Tamura, Motohide; Gaidos, Eric; Hirano, Teruyuki +13 more

Exoplanets in their infancy are ideal targets to probe the formation and evolution history of planetary systems, including the planet migration and atmospheric evolution and dissipation. In this paper, we present spectroscopic observations and analyses of two planetary transits of K2-33b, which is known to be one of the youngest transiting planets…

2024 Monthly Notices of the Royal Astronomical Society
XMM-Newton 5
A comparative high-resolution spectroscopic analysis of in situ and accreted globular clusters
DOI: 10.1051/0004-6361/202451377 Bibcode: 2024A&A...691A.226C

Massari, D.; Bellazzini, M.; Mucciarelli, A. +2 more

Globular clusters (GCs) are extremely intriguing systems that help in reconstructing the assembly of the Milky Way via the characterisation of their chemo-chrono-dynamical properties. In this study, we use high-resolution spectroscopic archival data from UVES and UVES-FLAMES at the VLT to compare the chemistry of GCs dynamically tagged as either G…

2024 Astronomy and Astrophysics
Gaia 5
On the existence of `Maia variables'
DOI: 10.1017/pasa.2024.76 Bibcode: 2024PASA...41...82K

Jayaraman, Rahul; Ozuyar, Dogus; Handler, Gerald +5 more

There are different classes of pulsating stars in the H-R diagram. While many of those classes are undisputed, some remain a mystery such as the objects historically called `Maia variables'. Whereas the presence of such a class was suggested seven decades ago, no pulsational driving mechanism is known that could excite short-period oscillations in…

2024 Publications of the Astronomical Society of Australia
Gaia 5
Beyond Point Masses. II. Non-Keplerian Shape Effects Are Detectable in Several TNO Binaries
DOI: 10.3847/1538-3881/ad26f0 Bibcode: 2024AJ....167..144P

Grundy, Will; Suggs, Christiana Z.; Proudfoot, Benjamin C. N. +60 more

About 40 trans-Neptunian binaries (TNBs) have fully determined orbits with about 10 others being solved except for breaking the mirror ambiguity. Despite decades of study, almost all TNBs have only ever been analyzed with a model that assumes perfect Keplerian motion (e.g., two point masses). In reality, all TNB systems are non-Keplerian due to no…

2024 The Astronomical Journal
eHST 5
Turbulence, and Proton and Electron Heating Rates in the Solar Corona: Analytical Approach
DOI: 10.3847/1538-4357/ad3109 Bibcode: 2024ApJ...966...52A

Telloni, Daniele; Zank, Gary P.; Adhikari, Laxman +5 more

Analytical solutions for 2D and slab turbulence energies in the solar corona are presented, including a derivation of the corresponding correlation lengths, with implications for the proton and electron temperatures in the solar corona. These solutions are derived by solving the transport equations for 2D and slab turbulence energies and their cor…

2024 The Astrophysical Journal
SolarOrbiter 5
WD 0141-675: a case study on how to follow-up astrometric planet candidates around white dwarfs
DOI: 10.1093/mnras/stad3098 Bibcode: 2024MNRAS.527..977R

Vanderburg, Andrew; Hermes, J. J.; Toonen, Silvia +22 more

This work combines spectroscopic and photometric data of the polluted white dwarf WD 0141-675, which has a now retracted astrometric super-Jupiter candidate, and investigates the most promising ways to confirm Gaia astrometric planetary candidates and obtain follow-up data. Obtaining precise radial velocity measurements for white dwarfs is challen…

2024 Monthly Notices of the Royal Astronomical Society
Gaia eHST 5
A Case Study of Gas Impacted by Black-hole Jets with the JWST: Outflows, Bow Shocks, and High Excitation of the Gas in the Galaxy IC 5063
DOI: 10.3847/1538-4357/ad89ba Bibcode: 2024ApJ...977..156D

Malkan, Matthew; Armus, Lee; Spinoglio, Luigi +8 more

We present James Webb Space Telescope MIRI data of the inner ∼3 × 2 kpc2 of the galaxy IC 5063, in which the jets of a supermassive black hole interact with the gaseous disk they are crossing. Jet-driven outflows were known to be initiated along or near the jet path and to modify the stability of molecular clouds, possibly altering thei…

2024 The Astrophysical Journal
JWST 5
Can early dark energy be probed by the high-redshift galaxy abundance?
DOI: 10.1093/mnras/stae1871 Bibcode: 2024MNRAS.533..860L

Gong, Yan; Wang, Xin; Liu, Weiyang +1 more

The analysis of the cosmic microwave background data acquired by the Atacama Cosmology Telescope and the large-scale ($\ell \lesssim 1300$) Planck Telescope show a preference for the early dark energy (EDE) theory, which was set to alleviate the Hubble tension of the $\Lambda$ cold dark matter ($\Lambda$CDM) model by decreasing the sound horizon $…

2024 Monthly Notices of the Royal Astronomical Society
eHST JWST 5
Investigating Model Dependencies for Obscured Active Galactic Nuclei: A Case Study of NGC 3982
DOI: 10.3847/1538-4357/ad3235 Bibcode: 2024ApJ...966..116K

Ricci, Claudio; Boorman, Peter G.; Kallová, Kristína

X-ray spectroscopy of heavily obscured active galactic nuclei (AGN) offers a unique opportunity to study the circumnuclear environment of accreting supermassive black holes. However, individual models describing the obscurer have unique parameter spaces that give distinct parameter posterior distributions when fit to the same data. To assess the i…

2024 The Astrophysical Journal
XMM-Newton 5