Search Publications

Prevalence of SED Turndown among Classical Be Stars: Are All Be Stars Close Binaries?
DOI: 10.3847/1538-4357/ab48e7 Bibcode: 2019ApJ...885..147K

Hallinan, G.; Klement, Robert; Carciofi, A. C. +16 more

Rapid rotation is a fundamental characteristic of classical Be stars and a crucial property allowing for the formation of their circumstellar disks. Past evolution in a mass and angular momentum transferring binary system offers a plausible solution to how Be stars attained their fast rotation. Although the subdwarf remnants of mass donors in such…

2019 The Astrophysical Journal
AKARI Gaia 63
The mass-to-light ratios and the star formation histories of disc galaxies
DOI: 10.1093/mnras/sty3223 Bibcode: 2019MNRAS.483.1496S

Lelli, Federico; Schombert, James; McGaugh, Stacy

We combine new data from the main sequence (M* versus SFR) of star-forming galaxies and galaxy colours (from GALEX to Spitzer) with a flexible stellar population scheme to deduce the mass-to-light ratio (Υ*) of star-forming galaxies from the SPARC and S4G samples. We find that the main sequence for galaxies, partic…

2019 Monthly Notices of the Royal Astronomical Society
eHST 63
Anisotropy of the Milky Way’s Stellar Halo Using K Giants from LAMOST and Gaia
DOI: 10.3847/1538-3881/aafd2e Bibcode: 2019AJ....157..104B

Bird, Sarah A.; Yang, Chengqun; Liu, Chao +3 more

The anisotropy parameter β characterizes the extent to which orbits in stellar systems are predominantly radial or tangential and is likely to constrain, for the stellar halo of the Milky Way, scenarios for its formation and evolution. We have measured β as a function of Galactocentric radius from 5 to 100 kpc for 7664 metal-poor ([Fe/H] < -1.3…

2019 The Astronomical Journal
Gaia 63
Major Mergers Are Not the Dominant Trigger for High-accretion AGNs at z ∼ 2
DOI: 10.3847/1538-4357/ab385b Bibcode: 2019ApJ...882..141M

Cohen, Seth; van der Wel, Arjen; Windhorst, Rogier A. +8 more

Research over the past decade has shown diminishing evidence for major galaxy mergers being a dominant mechanism for the growth of supermassive black holes (BHs) in galaxies and the triggering of optically or X-ray-selected active galactic nuclei (AGNs). For the first time we test whether such a connection exists at least in the most “plausible” p…

2019 The Astrophysical Journal
eHST 63
A Uniform Retrieval Analysis of Ultra-cool Dwarfs. III. Properties of Y Dwarfs
DOI: 10.3847/1538-4357/ab16db Bibcode: 2019ApJ...877...24Z

Line, Michael R.; Schneider, Adam C.; Patience, Jennifer +1 more

Ultra-cool brown dwarfs offer a unique window into understanding substellar atmospheric physics and chemistry. Their strong molecular absorption bands at infrared wavelengths, Jupiter-like radii, cool temperatures, and lack of complicating stellar irradiation make them ideal test beds for understanding Jovian-like atmospheres. Here, we report the …

2019 The Astrophysical Journal
eHST 63
Particle Acceleration at 5 au Associated with Turbulence and Small-scale Magnetic Flux Ropes
DOI: 10.3847/1538-4357/aafcb2 Bibcode: 2019ApJ...872....4Z

Chen, Y.; Zank, G. P.; Zhao, L. -L. +4 more

An observational analysis of an atypical energetic particle event near 5 au measured by the Ulysses spacecraft is presented. A previous study has attributed the unusual enhancement of energetic proton flux to the presence of small-scale dynamic magnetic islands or flux ropes. Here, we find that the generation of these magnetic islands may be relat…

2019 The Astrophysical Journal
Ulysses 63
GRB 161219B/SN 2016jca: a powerful stellar collapse
DOI: 10.1093/mnras/stz1588 Bibcode: 2019MNRAS.487.5824A

D'Avanzo, P.; Melandri, A.; Pian, E. +26 more

We report observations and analysis of the nearby gamma-ray burst GRB 161219B (redshift z = 0.1475) and the associated Type Ic supernova (SN) 2016jca. GRB 161219B had an isotropic gamma-ray energy of ∼1.6 × 1050 erg. Its afterglow is likely refreshed at an epoch preceding the first photometric points (0.6 d), which slows down the decay …

2019 Monthly Notices of the Royal Astronomical Society
eHST 63
Rotation and pulsation in Ap stars: first light results from TESS sectors 1 and 2
DOI: 10.1093/mnras/stz1332 Bibcode: 2019MNRAS.487.3523C

Handler, G.; Niemczura, E.; Suárez, J. C. +36 more

We present the first results from the Transiting Exoplanet Survey Satellite (TESS) on the rotational and pulsational variability of magnetic chemically peculiar A-type stars. We analyse TESS 2-min cadence data from sectors 1 and 2 on a sample of 83 stars. Five new rapidly oscillating Ap (roAp) stars are announced. One of these pulsates with period…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 62
ASASSN-18tb: a most unusual Type Ia supernova observed by TESS and SALT
DOI: 10.1093/mnras/stz1445 Bibcode: 2019MNRAS.487.2372V

Gromadzki, M.; Kochanek, C. S.; Stanek, K. Z. +16 more

We present photometric and spectroscopic observations of the unusual Type Ia supernova ASASSN-18tb, including a series of Southern African Large Telescope spectra obtained over the course of nearly six months and the first observations of a supernova by the Transiting Exoplanet Survey Satellite. We confirm a previous observation by Kollmeier et al…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 62
Discovery of Strongly Inverted Metallicity Gradients in Dwarf Galaxies at z ∼ 2
DOI: 10.3847/1538-4357/ab3861 Bibcode: 2019ApJ...882...94W

Schmidt, Kasper B.; Treu, Tommaso; Daddi, Emanuele +12 more

We report the first measurements with sub-kiloparsec spatial resolution of strongly inverted gas-phase metallicity gradients in two dwarf galaxies at z ∼ 2. The galaxies have stellar masses ∼109 {M}, specific star formation rate ∼20 Gyr-1, and global metallicity 12+{log}({{O}}/{{H}})∼ 8.1 (1/4 solar), assuming t…

2019 The Astrophysical Journal
eHST 62