Search Publications

Testing White Dwarf Age Estimates Using Wide Double White Dwarf Binaries from Gaia EDR3
DOI: 10.3847/1538-4357/ac78d9 Bibcode: 2022ApJ...934..148H

Hermes, J. J.; van Saders, Jennifer L.; El-Badry, Kareem +4 more

White dwarf (WD) stars evolve simply and predictably, making them reliable age indicators. However, self-consistent validation of the methods for determining WD total ages has yet to be widely performed. This work uses 1565 wide (>100 au) WD+WD binaries and 24 new triples containing at least two WDs to test the accuracy and validity of WD total…

2022 The Astrophysical Journal
Gaia 30
Rotation Distributions around the Kraft Break with TESS and Kepler: The Influences of Age, Metallicity, and Binarity
DOI: 10.3847/1538-4357/ac60a1 Bibcode: 2022ApJ...930....7A

Pan, Kaike; van Saders, Jennifer L.; Claytor, Zachary R. +6 more

Stellar rotation is a complex function of mass, metallicity, and age and can be altered by binarity. To understand the importance of these parameters in main-sequence stars, we have assembled a sample of observations that spans a range of these parameters using a combination of observations from The Transiting Exoplanet Survey Satellite (TESS) and…

2022 The Astrophysical Journal
Gaia 30
The extreme properties of the nearby hyper-Eddington accreting active galactic nucleus in IRAS 04416+1215
DOI: 10.1093/mnras/stab3152 Bibcode: 2022MNRAS.509.3599T

Ho, Luis C.; Ricci, Claudio; Tombesi, Francesco +6 more

The physical properties of the accretion flow and of the X-ray emitting plasma, in supermassive black holes accreting at extreme Eddington rates, are still very unclear. Here we present the analysis of simultaneous XMM-Newton and NuSTAR observations of the hyper-Eddington Seyfert 1 galaxy IRAS 04416+1215, carried out in 2020. The main goal of thes…

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 30
Multiplicity of Galactic luminous blue variable stars
DOI: 10.1051/0004-6361/202040062 Bibcode: 2022A&A...657A...4M

Gosset, E.; Lobel, A.; Sana, H. +7 more

Context. Luminous blue variables (LBVs) are characterised by strong photometric and spectroscopic variability. They are thought to be in a transitory phase between O-type stars on the main sequence and the Wolf-Rayet stage. Recent studies also evoked the possibility that they might be formed through binary interaction. Only a few are known in bina…

2022 Astronomy and Astrophysics
Gaia 30
The ELM Survey. IX. A Complete Sample of Low-mass White Dwarf Binaries in the SDSS Footprint
DOI: 10.3847/1538-4357/ac72ac Bibcode: 2022ApJ...933...94B

Gianninas, A.; Kilic, Mukremin; Kosakowski, Alekzander +1 more

We present the discovery of 17 double white dwarf (WD) binaries from our ongoing search for extremely low mass (ELM) < 0.3 M WDs, objects that form from binary evolution. Gaia parallax provides a new means of target selection that we use to evaluate our original ELM Survey selection criteria. Cross-matching the Gaia and Sloan Digit…

2022 The Astrophysical Journal
Gaia 30
The Gas-Star Formation Cycle in Nearby Star-forming Galaxies. II. Resolved Distributions of CO and Hα Emission for 49 PHANGS Galaxies
DOI: 10.3847/1538-4357/ac474f Bibcode: 2022ApJ...927....9P

Kruijssen, J. M. Diederik; Rosolowsky, Erik; Chevance, Mélanie +36 more

The relative distribution of molecular gas and star formation in galaxies gives insight into the physical processes and timescales of the cycle between gas and stars. In this work, we track the relative spatial configuration of CO and Hα emission at high resolution in each of our galaxy targets and use these measurements to quantify the distributi…

2022 The Astrophysical Journal
Gaia 30
Exoplanet Atmosphere Retrievals in 3D Using Phase Curve Data with ARCiS: Application to WASP-43b
DOI: 10.1051/0004-6361/202142800 Bibcode: 2022A&A...665A...2C

Chubb, Katy L.; Min, Michiel


Aims: Our goal is to create a retrieval framework which encapsulates the three-dimensional (3D) nature of exoplanet atmospheres, and to apply it to observed emission phase curve and transmission spectra of the `hot Jupiter' exoplanet WASP-43b.
Methods: We present our 3D framework, which is freely available as a stand-alone module from Gi…

2022 Astronomy and Astrophysics
eHST 30
TOI-530b: a giant planet transiting an M-dwarf detected by TESS
DOI: 10.1093/mnras/stab3708 Bibcode: 2022MNRAS.511...83G

Barclay, Thomas; Latham, David W.; Bedell, Megan +46 more

We report the discovery of TOI-530b, a transiting Saturn-like planet around an M0.5V dwarf, delivered by the Transiting Exoplanet Survey Satellite (TESS). The host star is located at a distance of 147.7 ± 0.6 pc with a radius of R* = 0.54 ± 0.03 R and a mass of M* = 0.53 ± 0.02 M. We verify the planeta…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 30
The K2-3 System Revisited: Testing Photoevaporation and Core-powered Mass Loss with Three Small Planets Spanning the Radius Valley
DOI: 10.3847/1538-3881/ac7807 Bibcode: 2022AJ....164..172D

Youngblood, Allison; Crossfield, Ian J. M.; Kreidberg, Laura +11 more

Multiplanet systems orbiting M dwarfs provide valuable tests of theories of small-planet formation and evolution. K2-3 is an early M dwarf hosting three small exoplanets (1.5-2.0 R ) at distances of 0.07-0.20 au. We measure the high-energy spectrum of K2-3 with HST/COS and XMM-Newton and use empirically driven estimates of Lyα and extr…

2022 The Astronomical Journal
Gaia XMM-Newton eHST 30
A Bayesian Population Model for the Observed Dust Attenuation in Galaxies
DOI: 10.3847/1538-4357/ac6c80 Bibcode: 2022ApJ...932...54N

Foreman-Mackey, Daniel; Leja, Joel; Hayward, Christopher C. +2 more

Dust plays a pivotal role in determining the observed spectral energy distribution (SED) of galaxies. Yet our understanding of dust attenuation is limited and our observations suffer from the dust-metallicity-age degeneracy in SED fitting (single galaxies), large individual variances (ensemble measurements), and the difficulty in properly dealing …

2022 The Astrophysical Journal
eHST 30