Search Publications

High-precision Dark Halo Virial Masses from Globular Cluster Numbers: Implications for Globular Cluster Formation and Galaxy Assembly
DOI: 10.3847/1538-3881/ab5b0e Bibcode: 2020AJ....159...56B

Forbes, Duncan A.; Burkert, Andreas

We confirm that the number of globular clusters (GCs), NGC, is an excellent tracer of their host galaxy's halo virial mass, Mvir. The simple linear relation Mvir = 5 × 109 M × NGC fits the data perfectly from Mvir = 1010 M to Mvir = 2 × …

2020 The Astronomical Journal
eHST 93
The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Multiband Constraints on Line-luminosity Functions and the Cosmic Density of Molecular Gas
DOI: 10.3847/1538-4357/abaa3b Bibcode: 2020ApJ...902..110D

Carilli, Chris; Inami, Hanae; Smail, Ian +20 more

We present a CO and atomic fine-structure line-luminosity function analysis using the ALMA Spectroscopic Survey (ASPECS) in the Hubble Ultra Deep Field. ASPECS consists of two spatially overlapping mosaics that cover the entire ALMA 3 mm and 1.2 mm bands. We combine the results of a line-candidate search of the 1.2 mm data cube with those previous…

2020 The Astrophysical Journal
eHST 93
A triple-star system with a misaligned and warped circumstellar disk shaped by disk tearing
DOI: 10.1126/science.aba4633 Bibcode: 2020Sci...369.1233K

Monnier, John D.; Schaefer, Gail H.; Lanthermann, Cyprien +29 more

Young stars are surrounded by a circumstellar disk of gas and dust, within which planet formation can occur. Gravitational forces in multiple star systems can disrupt the disk. Theoretical models predict that if the disk is misaligned with the orbital plane of the stars, the disk should warp and break into precessing rings, a phenomenon known as d…

2020 Science
Gaia 93
Cosmic dissonance: are new physics or systematics behind a short sound horizon?
DOI: 10.1051/0004-6361/201936720 Bibcode: 2020A&A...639A..57A

Treu, Tommaso; Fassnacht, Christopher D.; Birrer, Simon +12 more

Context. Persistent tension between low-redshift observations and the cosmic microwave background radiation (CMB), in terms of two fundamental distance scales set by the sound horizon rd and the Hubble constant H0, suggests new physics beyond the Standard Model, departures from concordance cosmology, or residual systematics. …

2020 Astronomy and Astrophysics
eHST 93
TESS Hunt for Young and Maturing Exoplanets (THYME). II. A 17 Myr Old Transiting Hot Jupiter in the Sco-Cen Association
DOI: 10.3847/1538-3881/ab94b7 Bibcode: 2020AJ....160...33R

Vanderburg, Andrew; Quinn, Samuel N.; Law, Nicholas M. +10 more

We present the discovery of a transiting hot Jupiter orbiting HIP 67522 (Teff ∼ 5650 K; M* ∼ 1.2M) in the 10-20 Myr old Sco-Cen OB association. We identified the transits in the TESS data using our custom notch filter planet search pipeline and characterize the system with additional photometry from Spitzer; spect…

2020 The Astronomical Journal
Gaia 93
Hot Exoplanet Atmospheres Resolved with Transit Spectroscopy (HEARTS). III. Atmospheric structure of the misaligned ultra-hot Jupiter WASP-121b
DOI: 10.1051/0004-6361/201936640 Bibcode: 2020A&A...635A.205B

Heng, K.; Ehrenreich, D.; Lendl, M. +21 more

Ultra-hot Jupiters offer interesting prospects for expanding our theories on dynamical evolution and the properties of extremely irradiated atmospheres. In this context, we present the analysis of new optical spectroscopy for the transiting ultra-hot Jupiter WASP-121b. We first refine the orbital properties of WASP-121b, which is on a nearly polar…

2020 Astronomy and Astrophysics
eHST 92
Debris Disk Results from the Gemini Planet Imager Exoplanet Survey's Polarimetric Imaging Campaign
DOI: 10.3847/1538-3881/ab9199 Bibcode: 2020AJ....160...24E

Matthews, Brenda C.; Duchêne, Gaspard; Esposito, Thomas M. +62 more

We report the results of a ∼4 yr direct imaging survey of 104 stars to resolve and characterize circumstellar debris disks in scattered light as part of the Gemini Planet Imager (GPI) Exoplanet Survey. We targeted nearby (≲150 pc), young (≲500 Myr) stars with high infrared (IR) excesses (LIR/L > 10-5), includin…

2020 The Astronomical Journal
Gaia Herschel eHST 92
The SPOTS Models: A Grid of Theoretical Stellar Evolution Tracks and Isochrones for Testing the Effects of Starspots on Structure and Colors
DOI: 10.3847/1538-4357/ab722e Bibcode: 2020ApJ...891...29S

Somers, Garrett; Pinsonneault, Marc H.; Cao, Lyra

One-dimensional stellar evolution models have been successful at representing the structure and evolution of stars in diverse astrophysical contexts, but complications have been noted in the context of young, magnetically active stars, as well as close binary stars with significant tidal interactions. Numerous puzzles are associated with pre-main-…

2020 The Astrophysical Journal
Gaia 91
The R-Process Alliance: Fourth Data Release from the Search for R-process-enhanced Stars in the Galactic Halo
DOI: 10.3847/1538-4365/ab9c19 Bibcode: 2020ApJS..249...30H

Grebel, Eva K.; Drout, Maria R.; Steinmetz, Matthias +22 more

This compilation is the fourth data release from the R-Process Alliance (RPA) search for r-process-enhanced stars and the second release based on "snapshot" high-resolution (R ∼ 30,000) spectra collected with the du Pont 2.5 m Telescope. In this data release, we propose a new delineation between the r-I and r-II stellar classes at $[\mathrm{Eu}/\m…

2020 The Astrophysical Journal Supplement Series
Gaia 91
GROWTH on S190814bv: Deep Synoptic Limits on the Optical/Near-infrared Counterpart to a Neutron Star-Black Hole Merger
DOI: 10.3847/1538-4357/ab6a1b Bibcode: 2020ApJ...890..131A

Cenko, S. Bradley; Kong, Albert K. H.; Gromadzki, Mariusz +49 more

On 2019 August 14, the Advanced LIGO and Virgo interferometers detected the high-significance gravitational wave (GW) signal S190814bv. The GW data indicated that the event resulted from a neutron star-black hole (NSBH) merger, or potentially a low-mass binary BH merger. Due to the low false-alarm rate and the precise localization (23 deg2

2020 The Astrophysical Journal
Gaia 91