Search Publications

New precise astrometric observations of Nereid in 2012-2017
DOI: 10.1016/j.pss.2018.01.001 Bibcode: 2018P&SS..152...82Y

Cheng, X.; Yan, D.; Qiao, R. C. +4 more

Nereid is one of the most distinctive natural satellites that we know in the Solar system. The orbit of Nereid is highly eccentric and inclined with respect to the equator of its primary, Neptune. Studying Nereid is one of the inspiring ways to acquire better knowledge of the Solar system. Due to its faintness, the ground-based observations of Ner…

2018 Planetary and Space Science
Gaia 11
An excitation mechanism for discrete chorus elements in the magnetosphere
DOI: 10.5194/angeo-36-1201-2018 Bibcode: 2018AnGeo..36.1201B

Bespalov, Peter; Savina, Olga

A beam pulsed amplifier mechanism responsible for effective amplification of short very low frequency (VLF) electromagnetic pulses is proposed. Effective amplification near the magnetic equator outside the plasmasphere is considered. A conditional growth rate of short electromagnetic pulses is calculated. Obtained results can explain some importan…

2018 Annales Geophysicae
Cluster 11
They Might Be Giants: An Efficient Color-based Selection of Red Giant Stars
DOI: 10.3847/2041-8213/aacdf1 Bibcode: 2018ApJ...861L..16C

Conroy, Charlie; Dotter, Aaron; Johnson, Benjamin D. +4 more

We present a color-based method for identifying red giants based on the Pan-STARRS grz and WISE W1 and W2 photometry. We utilize a subsample of bright stars with precise parallaxes from Gaia’s second data release (DR2) to verify that the color-based selection reliably separates dwarfs from giants. The selection is conservative in the sense that co…

2018 The Astrophysical Journal
Gaia 11
Constraining the nature of DG Tau A's thermal and non-thermal radio emission
DOI: 10.1093/mnras/sty2649 Bibcode: 2018MNRAS.481.5532P

Purser, S. J. D.; Ray, T. P.; Taylor, A. M. +3 more

DG Tau A, a class-II young stellar object (YSO), displays both thermal and non-thermal radio emission associated with its bipolar jet. To investigate the nature of this emission, we present sensitive (σ ∼ 2 {µ Jy} beam^{-1}), Karl G. Jansky Very Large Array (VLA) 6 and 10 GHz observations. Over 3.81 yr, no proper motion is observed towards t…

2018 Monthly Notices of the Royal Astronomical Society
Gaia 11
Cluster Observations of a Dispersive Flapping Event of Magnetotail Current Sheet
DOI: 10.1029/2018JA025196 Bibcode: 2018JGRA..123.5571R

Petrukovich, A. A.; Wei, Y.; Lui, A. T. Y. +5 more

A kink-like flapping event of Earth magnetotail current sheet, which consists of two frequency bands successively, is studied by the multipoint observations of Cluster. The multipoint analysis of Cluster observations demonstrates that the higher frequency band (period is about 10 min) has faster propagation velocity (about 30 km/s), shorter wavele…

2018 Journal of Geophysical Research (Space Physics)
Cluster 11
Particle simulation of electromagnetic emissions from electrostatic instability driven by an electron ring beam on the density gradient
DOI: 10.1063/1.5025912 Bibcode: 2018PhPl...25d2905H

Omura, Yoshiharu; Santolík, Ondřej; Horký, Miroslav

This paper presents the wave mode conversion between electrostatic and electromagnetic waves on the plasma density gradient. We use 2-D electromagnetic code KEMPO2 implemented with the generation of density gradient to simulate such a conversion process. In the dense region, we use ring beam instability to generate electron Bernstein waves and we …

2018 Physics of Plasmas
Cluster 11
IGR J19294+1816: a new Be-X-ray binary revealed through infrared spectroscopy
DOI: 10.1093/mnras/sty333 Bibcode: 2018MNRAS.476.2110R

Solano, E.; Torrejón, J. M.; Rodes-Roca, J. J. +2 more

The aim of this work is to characterize the counterpart to the INTErnational Gamma-Ray Astrophysics Laboratory high-mass X-ray binary candidate IGR J19294+1816 so as to establish its true nature. We obtained H-band spectra of the selected counterpart acquired with the Near Infrared Camera and Spectrograph instrument mounted on the Telescopio Nazio…

2018 Monthly Notices of the Royal Astronomical Society
Gaia 11
Angular Sizes and Effective Temperatures of O-type Stars from Optical Interferometry with the CHARA Array
DOI: 10.3847/1538-4357/aaec04 Bibcode: 2018ApJ...869...37G

Gies, Douglas R.; Schaefer, Gail H.; Hillier, D. John +3 more

We present interferometric observations of six O-type stars that were made with the Precision Astronomical Visible Observations beam combiner at the Center for High Angular Resolution Astronomy (CHARA) Array. The observations include multiple brackets for three targets, λ Ori A, ζ Oph, and 10 Lac, but there are only preliminary, single observation…

2018 The Astrophysical Journal
AKARI Gaia IUE eHST 11
Jeans that fit: weighing the mass of the Milky Way analogues in the ΛCDM universe
DOI: 10.1093/mnras/sty118 Bibcode: 2018MNRAS.475.4434K

Sharma, Sanjib; Driver, Simon P.; Robotham, Aaron S. G. +2 more

The spherical Jeans equation is a widely used tool for dynamical study of gravitating systems in astronomy. Here, we test its efficacy in robustly weighing the mass of Milky Way analogues, given they need not be in equilibrium or even spherical. Utilizing Milky Way stellar haloes simulated in accordance with Λ cold dark matter (ΛCDM) cosmology by …

2018 Monthly Notices of the Royal Astronomical Society
Gaia 11
Synthesis of Molecular Oxygen via Irradiation of Ice Grains in the Protosolar Nebula
DOI: 10.3847/1538-4357/aab6b9 Bibcode: 2018ApJ...858...66M

Wurz, P.; Lunine, J. I.; Danger, G. +4 more

Molecular oxygen has been detected in the coma of comet 67P/Churyumov-Gerasimenko with a mean abundance of 3.80 ± 0.85% by the ROSINA mass spectrometer on board the Rosetta spacecraft. To account for the presence of this species in comet 67P/Churyumov-Gerasimenko, it has been shown that the radiolysis of ice grain precursors of comets is a viable …

2018 The Astrophysical Journal
Rosetta 11