Search Publications

Weighing in on black hole binaries with BPASS: LB-1 does not contain a 70 M black hole
DOI: 10.1093/mnras/staa1324 Bibcode: 2020MNRAS.495.2786E

Steeghs, D. T. H.; Stanway, E. R.; Eldridge, J. J. +3 more

The recent identification of a candidate very massive (70 M) black hole (BH) is at odds with our current understanding of stellar winds and pair-instability supernovae. We investigate alternate explanations for this system by searching the BPASS v2.2 stellar and population synthesis models for those that match the observed properties o…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 55
A Terrestrial-mass Rogue Planet Candidate Detected in the Shortest-timescale Microlensing Event
DOI: 10.3847/2041-8213/abbfad Bibcode: 2020ApJ...903L..11M

Han, Cheongho; Udalski, Andrzej; Lee, Chung-Uk +29 more

Some low-mass planets are expected to be ejected from their parent planetary systems during early stages of planetary system formation. According to planet formation theories, such as the core accretion theory, typical masses of ejected planets should be between 0.3 and 1.0 M. Although in practice such objects do not emit any light, th…

2020 The Astrophysical Journal
Gaia 55
The tidal remnant of an unusually metal-poor globular cluster
DOI: 10.1038/s41586-020-2483-6 Bibcode: 2020Natur.583..768W

Lewis, Geraint F.; Casey, Andrew R.; Erkal, Denis +18 more

Globular clusters are some of the oldest bound stellar structures observed in the Universe1. They are ubiquitous in large galaxies and are believed to trace intense star-formation events and the hierarchical build-up of structure2,3. Observations of globular clusters in the Milky Way, and a wide variety of other galaxies, hav…

2020 Nature
Gaia 55
The Bulge Radial Velocity Assay for RR Lyrae Stars (BRAVA-RR) DR2: A Bimodal Bulge?
DOI: 10.3847/1538-3881/ab8d35 Bibcode: 2020AJ....159..270K

Rich, R. Michael; Kunder, Andrea; Wojno, Jennifer +11 more

The radial velocities of 2768 fundamental-mode RR Lyrae stars (RRLs) toward the southern Galactic bulge are presented, spanning the southern bulge from -8° < l < + 8° and -3° < b < -6°. Distances derived from the pulsation properties of the RRLs are combined with Gaia proper motions to give constraints on the orbital motions of 1389 RR…

2020 The Astronomical Journal
Gaia 54
Comparison of the Deep Atmospheric Dynamics of Jupiter and Saturn in Light of the Juno and Cassini Gravity Measurements
DOI: 10.1007/s11214-020-00705-7 Bibcode: 2020SSRv..216...84K

Stevenson, David J.; Iess, Luciano; Showman, Adam P. +4 more

The nature and structure of the observed east-west flows on Jupiter and Saturn have been a long-standing mystery in planetary science. This mystery has been recently unraveled by the accurate gravity measurements provided by the Juno mission to Jupiter and the Grand Finale of the Cassini mission to Saturn. These two experiments, which coincidental…

2020 Space Science Reviews
Cassini 54
Disentangling cataclysmic variables in Gaia's HR diagram
DOI: 10.1093/mnrasl/slz181 Bibcode: 2020MNRAS.492L..40A

López-Sanjuan, Carlos; Ederoclite, Alessandro; Schmidtobreick, Linda +1 more

Cataclysmic variables (CVs) are interacting binaries consisting of at least three components that control their colour and magnitude. Using Gaia, we here investigate the influence of the physical properties of these binaries on their position in the Hertzsprung-Russell (HR) diagram. The CVs are on average located between the main sequence and the …

2020 Monthly Notices of the Royal Astronomical Society
Gaia 54
HST Imaging of the Ionizing Radiation from a Star-forming Galaxy at z = 3.794
DOI: 10.3847/1538-4357/ab5fdc Bibcode: 2020ApJ...888..109J

Papovich, Casey; Castellano, Marco; Ferguson, Henry C. +17 more

We report on the Hubble Space Telescope (HST) detection of the Lyman-continuum (LyC) radiation emitted by a galaxy at redshift z = 3.794 dubbed Ion1. The LyC from Ion1 is detected at 820-890 Å with HST WFC3/UVIS in the F410M band (m410 = 27.60 ± 0.36 mAB, peak signal-to-noise ratio (S/N) = 4.17 in an r = 0"12 aperture) and 70…

2020 The Astrophysical Journal
eHST 54
PopSyCLE: A New Population Synthesis Code for Compact Object Microlensing Events
DOI: 10.3847/1538-4357/ab5fd3 Bibcode: 2020ApJ...889...31L

Hosek, Matthew W., Jr.; Lu, Jessica R.; Dawson, William A. +2 more

We present a new Milky Way microlensing simulation code, dubbed PopSyCLE (Population Synthesis for Compact object Lensing Events). PopSyCLE is the first resolved microlensing simulation to include a compact object distribution derived from numerical supernova explosion models and both astrometric and photometric microlensing effects. We demonstrat…

2020 The Astrophysical Journal
Gaia 54
Probing the Bright End of the Rest-frame Ultraviolet Luminosity Function at z = 8-10 with Hubble Pure-parallel Imaging
DOI: 10.3847/1538-4357/ab7659 Bibcode: 2020ApJ...891..146R

Finkelstein, Steven L.; Bagley, Micaela B.; Rojas-Ruiz, Sofía +5 more

Looking for bright galaxies born in the early universe is fundamental to investigating the Epoch of Reionization, the era when the first stars and galaxies ionized the intergalactic medium. We utilize Hubble Space Telescope pure-parallel imaging to select galaxy candidates at a time 500-650 million years after the Big Bang, which corresponds to re…

2020 The Astrophysical Journal
eHST 54
RedDots: a temperate 1.5 Earth-mass planet candidate in a compact multiterrestrial planet system around GJ 1061
DOI: 10.1093/mnras/staa248 Bibcode: 2020MNRAS.493..536D

Pallé, E.; Reiners, A.; Ribas, I. +16 more

Small low-mass stars are favourable targets for the detection of rocky habitable planets. In particular, planetary systems in the solar neighbourhood are interesting and suitable for precise characterization. The RedDots campaigns seek to discover rocky planets orbiting nearby low-mass stars. The 2018 campaign targeted GJ 1061, which is the 20th n…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 54