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Spacecraft Radio Frequency Fluctuations in the Solar Corona: A MESSENGER-HELIOS Composite Study
DOI: 10.3847/1538-4357/aaf6a8 Bibcode: 2019ApJ...871..202W

Wexler, David B.; Hollweg, Joseph V.; Jensen, Elizabeth A. +4 more

Fluctuations in plasma electron density may play a role in solar coronal energy transport and the dissipation of wave energy. Transcoronal spacecraft radio sounding observations reveal frequency fluctuations (FFs) that encode the electron number density disturbances, allowing an exploration of the coronal compressive wave and advected inhomogeneit…

2019 The Astrophysical Journal
SOHO 27
Flare and Warp of Galactic Disk with OB Stars from Gaia DR2
DOI: 10.3847/1538-4357/aafa17 Bibcode: 2019ApJ...871..208L

Zhao, Gang; Li, Chengdong; Yang, Chengqun +3 more

The OB stars are selected from the Gaia DR2 catalog to explore the flare and warp of the Galactic disk in this work. The Gaia and 2MASS photometric information is adopted as the criteria to choose the sample stars. We model the Galactic disk stellar distribution in this work taking the flare and warp into consideration. The parameters in the flare…

2019 The Astrophysical Journal
Gaia 27
Discovery of a very young high-mass X-ray binary associated with the supernova remnant MCSNR J0513-6724 in the LMC
DOI: 10.1093/mnras/stz2831 Bibcode: 2019MNRAS.490.5494M

Haberl, F.; Soszyński, I.; Udalski, A. +20 more

We report the discovery of a very young high-mass X-ray binary (HMXB) system associated with the supernova remnant (SNR) MCSNR J0513-6724 in the Large Magellanic Cloud (LMC), using XMM-Newton X-ray observations. The HMXB is located at the geometrical centre of extended soft X-ray emission, which we confirm as an SNR. The HMXB spectrum is consisten…

2019 Monthly Notices of the Royal Astronomical Society
XMM-Newton 27
Statistical Study on Multispacecraft Widespread Solar Energetic Particle Events During Solar Cycle 24
DOI: 10.1029/2019JA026832 Bibcode: 2019JGRA..124.6384X

St. Cyr, O. C.; Gopalswamy, N.; Mäkelä, P. +1 more

We conduct a statistical study on the large three-spacecraft widespread solar energetic particle (SEP) events. Longitudinal distributions of the peak intensities, onset delays, and relation between the SEP intensity, coronal mass ejection (CME) shock speed, width, and the kinetic energy of the CME have been investigated. We apply a Gaussian fit to…

2019 Journal of Geophysical Research (Space Physics)
SOHO 27
An Extremely Low-mass He White Dwarf Orbiting the Millisecond Pulsar J1342+2822B in the Globular Cluster M3
DOI: 10.3847/1538-4357/ab0e6b Bibcode: 2019ApJ...875...25C

Ferraro, F. R.; Lanzoni, B.; Pallanca, C. +3 more

We report on the discovery of the companion star to the millisecond pulsar J1342+2822B in the globular cluster M3. We exploited a combination of near-ultraviolet and optical observations acquired with the Hubble Space Telescope in order to search for the optical counterparts to the known millisecond pulsars in this cluster. At a position in excell…

2019 The Astrophysical Journal
Gaia eHST 27
[C I](1-0) and [C I](2-1) in Resolved Local Galaxies
DOI: 10.3847/1538-4357/ab4196 Bibcode: 2019ApJ...887..105C

Hunt, Leslie K.; Wilson, Christine D.; Rosolowsky, Erik +16 more

We present resolved [C I] line intensities of 18 nearby galaxies observed with the SPIRE FTS spectrometer on the Herschel Space Observatory. We use these data along with resolved CO line intensities from J up = 1 to 7 to interpret what phase of the interstellar medium the [C I] lines trace within typical local galaxies. A tight, linear …

2019 The Astrophysical Journal
Herschel 27
The Araucaria project: High-precision orbital parallax and masses of eclipsing binaries from infrared interferometry
DOI: 10.1051/0004-6361/201935837 Bibcode: 2019A&A...632A..31G

Weber, M.; Kervella, P.; Tkachenko, A. +9 more

Context. The precise determinations of stellar mass at ≲1% provide important constraints on stellar evolution models. Accurate parallax measurements can also serve as independent benchmarks for the next Gaia data release.
Aims: We measured the masses and distance of binary systems with a precision level better than 1% using a fully geometrica…

2019 Astronomy and Astrophysics
Gaia 27
Fractal statistics in young star clusters: structural parameters and dynamical evolution
DOI: 10.1093/mnras/stz2698 Bibcode: 2019MNRAS.490.2521H

Hetem, Annibal; Gregorio-Hetem, Jane

We used fractal statistics to quantify the degree of observed substructures in a sample of 50 embedded clusters and more evolved open clusters (< 100 Myr) found in different galactic regions. The observed fractal parameters were compared with N-body simulations from the literature, which reproduce star-forming regions under different initial co…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 27
The evolution of carbon-polluted white dwarfs at low effective temperatures
DOI: 10.1093/mnras/stz2915 Bibcode: 2019MNRAS.490.4166B

Blouin, Simon; Dufour, Patrick

Taking advantage of the Gaia Data Release 2, recent studies have revisited the evolution of carbon-polluted white dwarfs (DQs) across a large range of effective temperatures. These analyses have clearly confirmed the existence of two distinct DQ evolutionary sequences: one with normal-mass white dwarfs and one with heavily polluted and generally m…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 27
The angular momentum of disc galaxies at z = 1
DOI: 10.1051/0004-6361/201834456 Bibcode: 2019A&A...621L...6M

Fraternali, F.; Di Teodoro, E. M.; Oosterloo, T. +3 more

We investigate the relation between stellar mass (M) and specific stellar angular momentum (j), or "Fall relation", for a sample of 17 isolated, regularly rotating disc galaxies at z ∼ 1. All galaxies have rotation curves determined from Hα emission-line data; HST imaging in optical and infrared filters; and robust determin…

2019 Astronomy and Astrophysics
eHST 27