Search Publications

Mapping Metallicity Variations across Nearby Galaxy Disks
DOI: 10.3847/1538-4357/ab5115 Bibcode: 2019ApJ...887...80K

Chevance, M.; Meidt, S. E.; Schinnerer, E. +21 more

The distribution of metals within a galaxy traces the baryon cycle and the buildup of galactic disks, but the detailed gas phase metallicity distribution remains poorly sampled. We have determined the gas phase oxygen abundances for 7138 H II regions across the disks of eight nearby galaxies using Very Large Telescope/Multi Unit Spectroscopic Expl…

2019 The Astrophysical Journal
Gaia 152
A stellar census in globular clusters with MUSE: Binaries in NGC 3201
DOI: 10.1051/0004-6361/201936203 Bibcode: 2019A&A...632A...3G

Brinchmann, Jarle; Weilbacher, Peter M.; Kamann, Sebastian +8 more

We utilise multi-epoch MUSE spectroscopy to study binary stars in the core of the Galactic globular cluster NGC 3201. Our sample consists of 3553 stars with 54 883 spectra in total comprising 3200 main-sequence stars up to 4 magnitudes below the turn-off. Each star in our sample has between 3 and 63 (with a median of 14) reliable radial velocity m…

2019 Astronomy and Astrophysics
eHST 152
The mass of the Milky Way from satellite dynamics
DOI: 10.1093/mnras/stz365 Bibcode: 2019MNRAS.484.5453C

Grand, Robert J. J.; Gómez, Facundo A.; Marinacci, Federico +6 more

We present and apply a method to infer the mass of the Milky Way (MW) by comparing the dynamics of MW satellites to those of model satellites in the EAGLE cosmological hydrodynamics simulations. A distribution function (DF) for galactic satellites is constructed from EAGLE using specific angular momentum and specific energy, which are scaled so as…

2019 Monthly Notices of the Royal Astronomical Society
Gaia eHST 151
Constraining Primordial Black Hole Abundance with the Galactic 511 keV Line
DOI: 10.1103/PhysRevLett.123.251102 Bibcode: 2019PhRvL.123y1102D

DeRocco, William; Graham, Peter W.

Models in which dark matter consists entirely of primordial black holes (PBHs) with masses around 1 017 g are currently unconstrained. However, if PBHs are a component of the Galactic dark matter density, they will inject a large flux of energetic particles into the Galaxy as they radiate. Positrons produced by these black holes will su…

2019 Physical Review Letters
INTEGRAL 151
Do Kepler Superflare Stars Really Include Slowly Rotating Sun-like Stars?—Results Using APO 3.5 m Telescope Spectroscopic Observations and Gaia-DR2 Data
DOI: 10.3847/1538-4357/ab14e6 Bibcode: 2019ApJ...876...58N

Notsu, Yuta; Maehara, Hiroyuki; Namekata, Kosuke +7 more

We report the latest view of Kepler solar-type (G-type main-sequence) superflare stars, including recent updates with Apache Point Observatory (APO) 3.5 m telescope spectroscopic observations and Gaia-DR2 data. First, we newly conducted APO 3.5 m spectroscopic observations of 18 superflare stars found from Kepler 1-minute time-cadence data. More t…

2019 The Astrophysical Journal
Gaia 151
Kepler Planet Occurrence Rates for Mid-type M Dwarfs as a Function of Spectral Type
DOI: 10.3847/1538-3881/ab21d2 Bibcode: 2019AJ....158...75H

Muirhead, Philip S.; Cushing, Michael C.; Christiansen, Jessie L. +1 more

Previous studies of planet occurrence rates largely relied on photometric stellar characterizations. In this paper, we present planet occurrence rates for mid-type M dwarfs using spectroscopy, parallaxes, and photometry to determine stellar characteristics. Our spectroscopic observations have allowed us to constrain spectral type, temperatures, an…

2019 The Astronomical Journal
Gaia 150
Primordial black holes from inflation with nonminimal derivative coupling
DOI: 10.1103/PhysRevD.100.063532 Bibcode: 2019PhRvD.100f3532F

Wu, Puxun; Yu, Hongwei; Fu, Chengjie

We propose a novel enhancement mechanism of the curvature perturbations in the nonminimal derivative coupling inflation model with a coupling parameter related to the inflaton field. By considering a special form of the coupling parameter as a function of the inflaton, a period of ultra-slow-roll inflation can be realized due to the gravitationall…

2019 Physical Review D
INTEGRAL 150
The Streams of the Gaping Abyss: A Population of Entangled Stellar Streams Surrounding the Inner Galaxy
DOI: 10.3847/1538-4357/ab0080 Bibcode: 2019ApJ...872..152I

Malhan, Khyati; Ibata, Rodrigo A.; Martin, Nicolas F.

We present the discovery of a large population of stellar streams that surround the inner Galaxy, found in the Gaia DR2 catalog using the new STREAMFINDER algorithm. Here we focus on the properties of eight new high-significance structures found at heliocentric distances between 1 and 10 kpc and at Galactic latitudes | b| > 20^\circ , named Sli…

2019 The Astrophysical Journal
Gaia 149
Elemental and molecular abundances in comet 67P/Churyumov-Gerasimenko
DOI: 10.1093/mnras/stz2086 Bibcode: 2019MNRAS.489..594R

Mall, Urs; De Keyser, Johan; Hansen, Kenneth C. +18 more

Comets are considered to be some of the most pristine and unprocessed Solar system objects accessible to in situ exploration. Investigating their molecular and elemental composition takes us on a journey back to the early period of our Solar system and possibly even further. In this work, we deduce the bulk abundances of the major volatile species…

2019 Monthly Notices of the Royal Astronomical Society
Rosetta 149
The ASAS-SN catalogue of variable stars III: variables in the southern TESS continuous viewing zone
DOI: 10.1093/mnras/stz444 Bibcode: 2019MNRAS.485..961J

Kochanek, C. S.; Stanek, K. Z.; Dong, Subo +13 more

The All-Sky Automated Survey for Supernovae (ASAS-SN) provides long-baseline (∼4 yr) light curves for sources brighter than V ≲ 17 mag across the whole sky. The Transiting Exoplanet Survey Satellite (TESS) has started to produce high-quality light curves with a baseline of at least 27 d, eventually for most of the sky. The combination of ASAS-SN a…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 149