Search Publications

Probability of Forming Gaps in the GD-1 Stream by Close Encounters of Globular Clusters
DOI: 10.3847/1538-4357/aca090 Bibcode: 2022ApJ...941..129D

Hattori, Kohei; Doke, Yuka

One of the most intriguing properties of the GD-1 stellar stream is the existence of three gaps. If these gaps were formed by close encounters with dark matter subhalos, the GD-1 stream opens an exciting window through which we can see the size, mass, and velocity distributions of the dark matter subhalos in the Milky Way. However, in order to use…

2022 The Astrophysical Journal
Gaia 13
V456 Cyg: An eclipsing binary with tidally perturbed g-mode pulsations
DOI: 10.1051/0004-6361/202142833 Bibcode: 2022A&A...659A.177V

Southworth, J.; Bowman, D. M.; Van Reeth, T. +1 more

Context. Many well-known bright stars have been observed by the ongoing transiting exoplanet survey satellite (TESS) space mission. For several of them, these new data reveal previously unobserved variability, such as tidally perturbed pulsations in close binary stars.
Aims: Using newly detected gravity-mode (g-mode) pulsations in V456 Cyg, w…

2022 Astronomy and Astrophysics
Gaia 13
HAZMAT. VIII. A Spectroscopic Analysis of the Ultraviolet Evolution of K Stars: Additional Evidence for K Dwarf Rotational Stalling in the First Gigayear
DOI: 10.3847/1538-4357/ac5f48 Bibcode: 2022ApJ...929..169R

Loyd, R. O. Parke; Jackman, James A. G.; Barman, Travis +7 more

Efforts to discover and characterize habitable zone planets have primarily focused on Sun-like stars and M dwarfs. K stars, however, provide an appealing compromise between these two alternatives that has been relatively unexplored. Understanding the ultraviolet (UV) environment around such stars is critical to our understanding of their planets, …

2022 The Astrophysical Journal
Gaia eHST 13
DUVET: Spatially Resolved Observations of Star Formation Regulation via Galactic Outflows in a Starbursting Disk Galaxy
DOI: 10.3847/1538-4357/aca1bd Bibcode: 2022ApJ...941..163R

Fielding, Drummond; Cameron, Alex J.; Kacprzak, Glenn G. +14 more

We compare 500 pc scale, resolved observations of ionized and molecular gas for the z ~ 0.02 starbursting disk galaxy IRAS08339+6517, using measurements from KCWI and NOEMA. We explore the relationship of the star-formation-driven ionized gas outflows with colocated galaxy properties. We find a roughly linear relationship between the outflow mass …

2022 The Astrophysical Journal
eHST 13
On the Formation of Solar Wind and Switchbacks, and Quiet Sun Heating
DOI: 10.3847/1538-4357/ac3d88 Bibcode: 2022ApJ...926..138U

Tripathi, Durgesh; Upendran, Vishal

The solar coronal heating in quiet Sun (QS) and coronal holes (CHs), including solar wind formation, are intimately tied by magnetic field dynamics. Thus, a detailed comparative study of these regions is needed to understand the underlying physical processes. CHs are known to have subdued intensity and larger blueshifts in the corona. This work in…

2022 The Astrophysical Journal
IRIS 13
Project Hephaistos - I. Upper limits on partial Dyson spheres in the Milky Way
DOI: 10.1093/mnras/stac280 Bibcode: 2022MNRAS.512.2988S

Wright, Jason T.; Zackrisson, Erik; Korn, Andreas J. +2 more

Dyson spheres are hypothetical megastructures built by advanced extraterrestrial civilizations to harvest radiation energy from stars. Here, we combine optical data from Gaia DR2 with mid-infrared data from AllWISE to set the strongest upper limits to date on the prevalence of partial Dyson spheres within the Milky Way, based on their expected was…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 13
Revisiting a Disky Origin for the Faint Branch of the Sagittarius Stellar Stream
DOI: 10.3847/2041-8213/ac738c Bibcode: 2022ApJ...932L..14O

Errani, Raphaël; Famaey, Benoit; Ibata, Rodrigo +2 more

We investigate ways to produce the bifurcation observed in the stellar stream of the Sagittarius dwarf galaxy (Sgr). Our method consists of running N-body simulations of Sgr falling into the Milky Way for the last 3 Gyr, with added test particles on disk orbits that span a wide range of initial positions, energies, and angular momenta. We find tha…

2022 The Astrophysical Journal
Gaia 13
MHD study of the planetary magnetospheric response during extreme solar wind conditions: Earth and exoplanet magnetospheres applications
DOI: 10.1051/0004-6361/202141181 Bibcode: 2022A&A...659A..10V

Pantellini, F.; Zarka, P.; Varela, J. +3 more

Context. The stellar wind and the interplanetary magnetic field modify the topology of planetary magnetospheres. Consequently, the hazardous effect of the direct exposition to the stellar wind, for example, regarding the integrity of satellites orbiting the Earth or the habitability of exoplanets, depends upon the space weather conditions.
Ai…

2022 Astronomy and Astrophysics
Cluster 13
The stellar 'Snake' - I. Whole structure and properties
DOI: 10.1093/mnras/stac843 Bibcode: 2022MNRAS.513..503W

Fang, Min; Wang, Fan; Tian, Haijun +10 more

To complement our previous discovery of the young snake-like structure in the solar neighbourhood and reveal the structure's full extent, we build two samples of stars within the Snake and its surrounding territory from Gaia Early Data Release 3 (EDR3). With the friends-of-friends algorithm, we identify 2694 and 9052 Snake member candidates from t…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 13
Molecular gas properties of Planck-selected protocluster candidates at z ≃ 1.3-3
DOI: 10.1051/0004-6361/202142255 Bibcode: 2022A&A...662A..85P

Kneissl, R.; Dole, H.; Frye, B. L. +3 more

We report on IRAM 30-m/EMIR observations of 38 Herschel sources chosen as the brightest red submillimeter (submm) sources in 18 Planck-selected fields drawn from the Planck high-z (PHz) sample of protocluster candidates. These fields host overdensities of red Herschel sources, with high star formation rates (∼10 000 M yr−1),…

2022 Astronomy and Astrophysics
Herschel 13