Search Publications

The MOSDEF Survey: A Census of AGN-driven Ionized Outflows at z = 1.4-3.8
DOI: 10.3847/1538-4357/ab4a7c Bibcode: 2019ApJ...886...11L

Siana, Brian; Azadi, Mojegan; Aird, James +13 more

Using data from the MOSFIRE Deep Evolution Field (MOSDEF) survey, we present a census of active galactic nucleus (AGN)-driven ionized outflows in a sample of 159 AGNs at 1.4 ≤ z ≤ 3.8. The sample spans AGN bolometric luminosities of 1044-47 erg s-1 and includes both quiescent and star-forming galaxies extending across 3 order…

2019 The Astrophysical Journal
eHST 70
The Peculiar Volatile Composition of CO-dominated Comet C/2016 R2 (PanSTARRS)
DOI: 10.3847/1538-3881/ab32e4 Bibcode: 2019AJ....158..128M

Villanueva, Geronimo L.; Cochran, Anita L.; Bauer, James +14 more

Comet C/2016 R2 (PanSTARRS) has a peculiar volatile composition, with CO being the dominant volatile, as opposed to H2O, and one of the largest N2/CO ratios ever observed in a comet. Using observations obtained with the Spitzer Space Telescope, NASA’s Infrared Telescope Facility, the 3.5 m Astrophysical Research Consortium te…

2019 The Astronomical Journal
AKARI 70
Proper Motions of Stellar Streams Discovered in the Dark Energy Survey
DOI: 10.3847/1538-4357/ab44bf Bibcode: 2019ApJ...885....3S

Wang, M. Y.; Kuehn, K.; Li, T. S. +14 more

We cross-match high-precision astrometric data from Gaia DR2 with accurate multiband photometry from the Dark Energy Survey (DES) DR1 to confidently measure proper motions for nine stellar streams in the DES footprint: Aliqa Uma, ATLAS, Chenab, Elqui, Indus, Jhelum, Phoenix, Tucana III, and Turranburra. We determine low-confidence proper-motion me…

2019 The Astrophysical Journal
Gaia 69
Linking galaxy structural properties and star formation activity to black hole activity with IllustrisTNG
DOI: 10.1093/mnras/stz102 Bibcode: 2019MNRAS.484.4413H

Somerville, Rachel S.; Torrey, Paul; Vogelsberger, Mark +11 more

We study the connection between active galactic nuclei (AGN) and their host galaxies through cosmic time in the large-scale cosmological IllustrisTNG simulations. We first compare BH properties, i.e. the hard X-ray BH luminosity function, AGN galaxy occupation fraction, and distribution of Eddington ratios, to available observational constraints. …

2019 Monthly Notices of the Royal Astronomical Society
eHST 69
Relative Alignment between the Magnetic Field and Molecular Gas Structure in the Vela C Giant Molecular Cloud Using Low- and High-density Tracers
DOI: 10.3847/1538-4357/ab1eb0 Bibcode: 2019ApJ...878..110F

Ward-Thompson, Derek; Fissel, Laura M.; Friesen, Rachel +37 more

We compare the magnetic field orientation for the young giant molecular cloud Vela C inferred from 500 µm polarization maps made with the BLASTPol balloon-borne polarimeter to the orientation of structures in the integrated line emission maps from Mopra observations. Averaging over the entire cloud we find that elongated structures in integr…

2019 The Astrophysical Journal
Gaia 69
Whistler Fan Instability Driven by Strahl Electrons in the Solar Wind
DOI: 10.3847/2041-8213/ab01bd Bibcode: 2019ApJ...871L..29V

Bale, S. D.; Krasnoselskikh, V.; Mozer, F. S. +3 more

We present a theoretical analysis of electron heat flux inhibition in the solar wind when a significant portion of the heat flux is carried by strahl electrons. We adopt core-strahl velocity distribution functions typical for the solar wind at 0.3-4 au to demonstrate that strahl electrons are capable of generating highly oblique whistler waves at …

2019 The Astrophysical Journal
Cluster 69
The Type II-plateau Supernova 2017eaw in NGC 6946 and Its Red Supergiant Progenitor
DOI: 10.3847/1538-4357/ab1136 Bibcode: 2019ApJ...875..136V

Van Dyk, Schuyler D.; Filippenko, Alexei V.; Kelly, Patrick L. +31 more

We present extensive optical photometric and spectroscopic observations, from 4 to 482 days after explosion, of the Type II-plateau (II-P) supernova (SN) 2017eaw in NGC 6946. SN 2017eaw is a normal SN II-P intermediate in properties between, for example, SN 1999em and SN 2012aw and the more luminous SN 2004et, also in NGC 6946. We have determined …

2019 The Astrophysical Journal
eHST 69
The refractory-to-ice mass ratio in comets
DOI: 10.1093/mnras/sty2926 Bibcode: 2019MNRAS.482.3326F

Blum, J.; Gundlach, B.; Mottola, S. +6 more

We review the complex relationship between the dust-to-gas mass ratio usually estimated in the material lost by comets, and the refractory-to-ice mass ratio inside the nucleus, which constrains the origin of comets. Such a relationship is dominated by the mass transfer from the perihelion erosion to fallout over most of the nucleus surface. This m…

2019 Monthly Notices of the Royal Astronomical Society
Rosetta 69
WASP-4b Arrived Early for the TESS Mission
DOI: 10.3847/1538-3881/ab189f Bibcode: 2019AJ....157..217B

Dai, F.; Winn, J. N.; Jenkins, J. M. +21 more

The Transiting Exoplanet Survey Satellite (TESS) recently observed 18 transits of the hot Jupiter WASP-4b. The sequence of transits occurred 81.6 ± 11.7 s earlier than had been predicted, based on data stretching back to 2007. This is unlikely to be the result of a clock error, because TESS observations of other hot Jupiters (WASP-6b, 18b, and 46b…

2019 The Astronomical Journal
Gaia 69
A quantitative analysis of systematic differences in the positions and proper motions of Gaia DR2 with respect to VLBI
DOI: 10.1093/mnras/sty2807 Bibcode: 2019MNRAS.482.3023P

Petrov, L.; Kovalev, Y. Y.; Plavin, A. V.

We have analysed the differences in positions of 9081 matched sources between the Gaia Data Release 2 (DR2) and very long baseline interferometry (VLBI) catalogues. The median position uncertainty of matched sources in the VLBI catalogue is a factor of two larger than the median position uncertainty in Gaia DR2. There are 9 per cent matched source…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 69