Search Publications

Radial Velocity Comparison of Gaia DR2 and RAVE DR5 Survey: A Systematic Offset in Radial Velocities among a Group of Highly Accurate Radial Velocity Stars
DOI: 10.3847/1538-3881/aadcde Bibcode: 2018AJ....156..170D

Deepak; Reddy, Bacham E.

Here, we report a comparative study of radial velocity (RV) data of two major surveys: Gaia Data Release 2 and RAVE Data Release 5. We restricted the sample to stars with relatively accurate RVs ({σ }RV}{Gaia}}≤slant 2 km s-1 or ≤2%, and {σ }RV}RAVE}}≤slant 2 km s-1 or ≤2%). The dif…

2018 The Astronomical Journal
Gaia 5
Probing Strong Binary Interactions and Accretion in AGB Stars with the ngVLA
Bibcode: 2018ASPC..517..403S

Sahai, R.

Understanding strong binary interactions is of wide astrophysical importance, and the deaths of most stars in the Universe that evolve in a Hubble time could be fundamentally affected by such interactions. These stars end their lives, evolving from Asymptotic Giant Branch (AGB) stars with extensive mass-loss into planetary nebulae with a spectacul…

2018 Science with a Next Generation Very Large Array
XMM-Newton 4
Intermittency spectra of current helicity in solar active regions
DOI: 10.1093/mnras/sty2109 Bibcode: 2018MNRAS.480.3780K

Zhang, Hongqi; Abramenko, V. I.; Kuzanyan, K. M. +2 more

We analyse the spatial distribution of current helicity in solar active regions. A comparison of current helicity maps derived from three different instruments (Helioseismic and Magnetic Imager on board the Solar Dynamics Observatory, SDO/HMI, Spectro-Polarimeter on board the Hinode, and Solar Magnetic Field Telescope at the Huairou Solar Observin…

2018 Monthly Notices of the Royal Astronomical Society
Hinode 4
Polarimetric and spectroscopic study of radio-quiet weak emission line quasars
DOI: 10.1093/mnras/sty1802 Bibcode: 2018MNRAS.479.5075K

Stalin, C. S.; Petitjean, P.; Srianand, R. +3 more

A small subset of optically selected radio-quiet quasars showing weak or no emission lines may turn out to be the elusive radio-quiet BL Lac objects, or simply be radio-quiet QSOs with a still-forming/shielded broad line region (BLR). High polarization (p > 3-4 per cent), a hallmark of BL Lacs, can be used to test whether some optically selecte…

2018 Monthly Notices of the Royal Astronomical Society
Gaia 4
Non-Gaussianity and cross-scale coupling in interplanetary magnetic field turbulence during a rope-rope magnetic reconnection event
DOI: 10.5194/angeo-36-497-2018 Bibcode: 2018AnGeo..36..497M

Miranda, Rodrigo A.; Chian, Abraham C. -L.; Schelin, Adriane B. +1 more

In a recent paper (Chian et al., 2016) it was shown that magnetic reconnection at the interface region between two magnetic flux ropes is responsible for the genesis of interplanetary intermittent turbulence. The normalized third-order moment (skewness) and the normalized fourth-order moment (kurtosis) display a quadratic relation with a parabolic…

2018 Annales Geophysicae
Cluster 4
Multilayer mirror-based soft x-ray polarimeter for astronomical observations
DOI: 10.1117/1.JATIS.4.1.011002 Bibcode: 2018JATIS...4a1002P

Marshall, Herman L.; Narendranath, Shyama; Panini, Singam S. +3 more

A simple design of a soft x-ray polarimeter using multilayer mirrors is presented. A multilayer mirror acts as a linear polarization analyzer for x-rays at incidence angles close to the Brewster angle. The instrument consists of an x-ray concentrator, a set of multilayer mirrors placed at 45 deg from the optical axis, and a detector at Nasmyth foc…

2018 Journal of Astronomical Telescopes, Instruments, and Systems
XMM-Newton 4
Statistical survey of day-side magnetospheric current flow using Cluster observations: bow shock
DOI: 10.5194/angeo-36-1073-2018 Bibcode: 2018AnGeo..36.1073L

Glassmeier, Karl-Heinz; Liebert, Evelyn; Nabert, Christian

We present the first comprehensive statistical survey of the day-side terrestrial bow shock current system based on a large number of Cluster spacecraft bow shock crossings. Calculating the 3-D current densities using fluxgate magnetometer data and the curlometer technique enables the investigation of current locations, directions, and magnitudes …

2018 Annales Geophysicae
Cluster 4
In-flight performance of the Canadian Astro-H Metrology System
DOI: 10.1117/1.JATIS.4.2.021405 Bibcode: 2018JATIS...4b1405G

Ishida, Manabu; Iizuka, Ryo; Gallo, Luigi C. +11 more

The Canadian Astro-H Metrology System (CAMS) on the Hitomi x-ray satellite is a laser alignment system that measures the lateral displacement (X/Y) of the extensible optical bench (EOB) along the optical axis of the hard x-ray telescopes (HXTs). The CAMS consists of two identical units that together can be used to discern translation and rotation …

2018 Journal of Astronomical Telescopes, Instruments, and Systems
Hitomi 4
Verification of Photometric Parallaxes with Gaia DR2 Data
DOI: 10.3390/galaxies7010007 Bibcode: 2018Galax...7....7M

Zhao, Gang; Karpov, Sergey; Sytov, Alexey +10 more

Results of comparison of Gaia DR2 parallaxes with data derived from a combined analysis of 2MASS (Two Micron All-Sky Survey), SDSS (Sloan Digital Sky Survey), GALEX (Galaxy Evolution Explorer), and UKIDSS (UKIRT Infrared Deep Sky Survey) surveys in four selected high-latitude |b|> 48° sky areas are presented. It is shown that multicolor photome…

2018 Galaxies
Gaia 4
Global structure of the heliosphere: 3D kinetic-MHD model and the interpretation of spacecraft data
DOI: 10.3367/UFNe.2017.04.038293 Bibcode: 2018PhyU...61..793I

Izmodenov, V. V.

This paper is a brief overview of research into the interaction between the solar wind and local interstellar medium. This interaction determines the global structure of the heliosphere (the region occupied by the solar wind) and has a complex multicomponent character. We describe the three-dimensional kinetic-magnetohydrodynamic model of the inte…

2018 Physics Uspekhi
Ulysses 4