Search Publications

Gastro Library. I. The Simulated Chemodynamical Properties of Several Gaia-Sausage-Enceladus-like Stellar Halos
DOI: 10.3847/1538-4357/ac8b0d Bibcode: 2022ApJ...937...12A

Laporte, Chervin F. P.; Debattista, Victor P.; Amarante, João A. S. +2 more

The Milky Way (MW) stellar halo contains relics of ancient mergers that tell the story of our galaxy's formation. Some of them are identified due to their similarity in energy, actions, and chemistry, referred to as the "chemodynamical space," and are often attributed to distinct merger events. It is also known that our galaxy went through a signi…

2022 The Astrophysical Journal
Gaia 53
Probing the Physics of the Solar Atmosphere with the Multi-slit Solar Explorer (MUSE). I. Coronal Heating
DOI: 10.3847/1538-4357/ac4222 Bibcode: 2022ApJ...926...52D

Matsumoto, Takuma; Polito, Vanessa; Golub, Leon +24 more

The Multi-slit Solar Explorer (MUSE) is a proposed mission composed of a multislit extreme ultraviolet (EUV) spectrograph (in three spectral bands around 171 Å, 284 Å, and 108 Å) and an EUV context imager (in two passbands around 195 Å and 304 Å). MUSE will provide unprecedented spectral and imaging diagnostics of the solar corona at high spatial …

2022 The Astrophysical Journal
IRIS 53
The pattern speed of the Milky Way bar/bulge from VIRAC and Gaia
DOI: 10.1093/mnras/stac603 Bibcode: 2022MNRAS.512.2171C

Gerhard, Ortwin; Clarke, Jonathan P.

We compare distance resolved, absolute proper motions in the Milky Way bar/bulge region to a grid of made-to-measure dynamical models with well-defined pattern speeds. The data are obtained by combining the relative VVV InfraRed Astrometric Catalogue (VIRAC) v1 proper motions with the Gaia Data Release 2 absolute reference frame. We undertake a co…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 53
Exploring the AGN-Ram Pressure Stripping Connection in Local Clusters
DOI: 10.3847/1538-4357/ac4225 Bibcode: 2022ApJ...927..130P

Fritz, Jacopo; Vulcani, Benedetta; Poggianti, Bianca M. +8 more

Ram pressure stripping (RPS) by the intracluster medium is one of the most advocated mechanisms that affect the properties of cluster galaxies. A recent study based on a small sample has found that many galaxies showing strong signatures of RPS also possess an active galactic nucleus (AGN), suggesting a possible correlation between the two phenome…

2022 The Astrophysical Journal
XMM-Newton 53
How Many Elements Matter?
DOI: 10.3847/1538-4357/ac5023 Bibcode: 2022ApJ...927..209T

Ting, Yuan-Sen; Weinberg, David H.

Some studies of stars' multielement abundance distributions suggest at least 5-7 significant dimensions, but others show that many elemental abundances can be predicted to high accuracy from [Fe/H] and [Mg/Fe] (or [Fe/H] and age) alone. We show that both propositions can be, and are, simultaneously true. We adopt a machine-learning technique known…

2022 The Astrophysical Journal
Gaia 53
Theory of Cosmic Ray Transport in the Heliosphere
DOI: 10.1007/s11214-022-00896-1 Bibcode: 2022SSRv..218...33E

Rankin, J. S.; Potgieter, M. S.; Ruffolo, D. +6 more

Modelling the transport of cosmic rays (CRs) in the heliosphere represents a global challenge in the field of heliophysics, in that such a study, if it were to be performed from first principles, requires the careful modelling of both large scale heliospheric plasma quantities (such as the global structure of the heliosphere, or the heliospheric m…

2022 Space Science Reviews
Ulysses 53
Extremely Low Mass Ratio Contact Binaries. I. The First Photometric and Spectroscopic Investigations of Ten Systems
DOI: 10.3847/1538-3881/ac8ff2 Bibcode: 2022AJ....164..202L

Li, Kai; Gao, Xing; Chen, Xu +4 more

The photometric and spectroscopic investigations of ten contact binaries were presented for the first time. It is discovered that the mass ratios of all the ten targets are smaller than 0.15, they are extremely low mass ratio contact binaries. Seven of them are deep contact binaries, two are medium contact binaries, while only one is a shallow con…

2022 The Astronomical Journal
Gaia 53
No Evidence for Axions from Chandra Observation of the Magnetic White Dwarf RE J0317-853
DOI: 10.1103/PhysRevLett.128.071102 Bibcode: 2022PhRvL.128g1102D

Safdi, Benjamin R.; Dessert, Christopher; Long, Andrew J.

Axions with couplings ga γ γ∼few ×10-11 GeV-1 to electromagnetism may resolve a number of astrophysical anomalies, such as unexpected ∼TeV transparency, anomalous stellar cooling, and x-ray excesses from nearby neutron stars. We show, however, that such axions are severely constrained by the nonobservation of x ray…

2022 Physical Review Letters
Gaia 53
Systematic Errors as a Source of Mass Discrepancy in Black Hole Microlensing Event OGLE-2011-BLG-0462
DOI: 10.3847/2041-8213/ac90bb Bibcode: 2022ApJ...937L..24M

Udalski, Andrzej; Gould, Andrew; Mróz, Przemek

Two independent groups reported the discovery of an isolated dark stellar remnant in the microlensing event OGLE-2011-BLG-0462 based on photometric ground-based observations coupled with astrometric measurements taken with the Hubble Space Telescope. These two analyses yielded discrepant mass measurements, with the first group reporting that the l…

2022 The Astrophysical Journal
eHST 53
The Featureless HST/WFC3 Transmission Spectrum of the Rocky Exoplanet GJ 1132b: No Evidence for a Cloud-free Primordial Atmosphere and Constraints on Starspot Contamination
DOI: 10.3847/1538-3881/ac75de Bibcode: 2022AJ....164...59L

Désert, Jean-Michel; Rackham, Benjamin V.; Morley, Caroline V. +10 more

Orbiting an M dwarf 12 pc away, the transiting exoplanet GJ 1132b is a prime target for transmission spectroscopy. With a mass of 1.7 M and radius of 1.1 R , GJ 1132b's bulk density indicates that this planet is rocky. Yet with an equilibrium temperature of 580 K, GJ 1132b may still retain some semblance of an atmosphere. …

2022 The Astronomical Journal
eHST 52