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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
ALMA 200 pc Resolution Imaging of Smooth Cold Dusty Disks in Typical z ∼ 3 Star-forming Galaxies
DOI: 10.3847/1538-4357/ab3791 Bibcode: 2019ApJ...882..107R

Daddi, E.; Elbaz, D.; Franco, M. +14 more

We present high-fidelity, 30 mas (200 pc) resolution ALMA rest-frame 240 µm observations of cold dust emission in three typical main-sequence star-forming galaxies (SFGs) at z ∼ 3 in the Hubble Ultra-Deep Field (HUDF). The cold dust is distributed within the smooth disklike central regions of star formation 1-3 kpc in diameter, despite their…

2019 The Astrophysical Journal
eHST 69
No evidence for intermediate-mass black holes in the globular clusters ω Cen and NGC 6624
DOI: 10.1093/mnras/stz2060 Bibcode: 2019MNRAS.488.5340B

Dreizler, S.; Usher, C.; Kamann, S. +8 more

We compare the results of a large grid of N-body simulations with the surface brightness and velocity dispersion profiles of the globular clusters ω Cen and NGC 6624. Our models include clusters with varying stellar-mass black hole retention fractions and varying masses of a central intermediate-mass black hole (IMBH). We find that an ∼ 45 000 M

2019 Monthly Notices of the Royal Astronomical Society
eHST 69
Two new free-floating or wide-orbit planets from microlensing
DOI: 10.1051/0004-6361/201834557 Bibcode: 2019A&A...622A.201M

Kaspi, Shai; Maoz, Dan; Han, Cheongho +57 more

Planet formation theories predict the existence of free-floating planets that have been ejected from their parent systems. Although they emit little or no light, they can be detected during gravitational microlensing events. Microlensing events caused by rogue planets are characterized by very short timescales tE (typically below two da…

2019 Astronomy and Astrophysics
Gaia 68
Searching for Highly Magnified Stars at Cosmological Distances: Discovery of a Redshift 0.94 Blue Supergiant in Archival Images of the Galaxy Cluster MACS J0416.1-2403
DOI: 10.3847/1538-4357/ab297d Bibcode: 2019ApJ...881....8C

Filippenko, Alexei V.; Foley, Ryan J.; Kelly, Patrick L. +12 more

Individual highly magnified stars have been recently discovered at lookback times of more than half the age of the universe, in lensed galaxies that straddle the critical curves of massive galaxy clusters. Having established their detectability, it is now important to carry out systematic searches for them in order to establish their frequency, an…

2019 The Astrophysical Journal
eHST 68
The evolutionary status of Cataclysmic Variables: eclipse modelling of 15 systems
DOI: 10.1093/mnras/stz976 Bibcode: 2019MNRAS.486.5535M

Knigge, C.; Gänsicke, B. T.; Dhillon, V. S. +13 more

We present measurements of the component masses in 15 Cataclysmic Variables (CVs) - 6 new estimates and 9 improved estimates. We provide new calibrations of the relationship between superhump period excess and mass ratio, and use this relation to estimate donor star masses for 225 superhumping CVs. With an increased sample of donor masses we revis…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 68