Search Publications

A Suzaku X-ray study of the mixed-morphology supernova remnant Kes 69 and searching for its gamma-ray counterpart
DOI: 10.1093/mnras/sty2387 Bibcode: 2018MNRAS.481.1416S

Sezer, A.; Yamazaki, R.; Ergin, T. +2 more

Kes 69 is a mixed-morphology (MM) supernova remnant (SNR) that is known to be interacting with molecular clouds based on 1720 MHz hydroxyl (OH) maser emission observations in the northeastern and southeastern regions. We present an investigation of Kes 69 using ∼67 ks Suzaku observation. The X-ray spectrum of the whole SNR is well fitted by a non-…

2018 Monthly Notices of the Royal Astronomical Society
Suzaku 5
SMHASH: a new mid-infrared RR Lyrae distance determination for the Local Group dwarf spheroidal galaxy Sculptor
DOI: 10.1093/mnras/sty2222 Bibcode: 2018MNRAS.481..578G

Majewski, Steven R.; Madore, Barry F.; Freedman, Wendy L. +12 more

We present a new distance estimation for the Milky Way dwarf spheroidal satellite Sculptor obtained from multi-epoch mid-infrared observations of RR Lyrae stars (RRLs). The 3.6 µm observations have been acquired with the Infrared Array Camera onboard the Spitzer Space Telescope as part of the SMHASH program. Mid-infrared light curves for 42 …

2018 Monthly Notices of the Royal Astronomical Society
Gaia 5
Probing the dynamical state, baryon content, and multiphase nature of galaxy clusters with bright background QSOs
DOI: 10.1093/mnras/sty2492 Bibcode: 2018MNRAS.481.4111G

Tripp, Todd M.; Burchett, Joseph N.; Wang, Q. Daniel +5 more

We have initiated a programme to study the physical/dynamical state of gas in galaxy clusters and the impact of the cluster environment on gaseous haloes of individual galaxies using X-ray imaging and UV absorption line spectroscopy of background QSOs. Here, we report results from the analysis Chandra and XMM-Newton archival data of five galaxy cl…

2018 Monthly Notices of the Royal Astronomical Society
XMM-Newton eHST 5
Changes in the pulse phase dependence of X-ray emission lines in 4U 1626-67 with a torque reversal
DOI: 10.1093/mnras/stx3121 Bibcode: 2018MNRAS.475..999B

Paul, Biswajit; Beri, Aru; Dewangan, Gulab C.

We report results from an observation with the XMM-Newton observatory of a unique X-ray pulsar 4U 1626-67. European Photon Imaging Camera-pn data during the current spin-up phase of 4U 1626-67 have been used to study pulse phase dependence of low-energy emission lines. We found strong variability of low-energy emission line at 0.915 keV with the p…

2018 Monthly Notices of the Royal Astronomical Society
XMM-Newton 5
3D mapping of the neutral X-ray absorption in the local interstellar medium: the Gaia and XMM-Newton synergy
DOI: 10.1093/mnras/sty1738 Bibcode: 2018MNRAS.479.3715G

Wilms, J.; García, Javier A.; Kallman, Timothy R. +4 more

We present a three-dimensional map of the hydrogen density distribution in the Galactic interstellar medium. The hydrogen-equivalent column densities were obtained from the Exploring the X-ray Transient and variable Sky project (EXTRAS) which provides equivalent NH values from X-ray spectral fits of observations within the XMM-Newton Da…

2018 Monthly Notices of the Royal Astronomical Society
Gaia 5
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
Thermophysical modelling for high-resolution digital terrain models
DOI: 10.1093/mnras/sty1009 Bibcode: 2018MNRAS.478..386P

Pelivan, I.

A method is presented for efficiently calculating surface temperatures for highly resolved celestial body shapes. A thorough investigation of the necessary conditions leading to reach model convergence shows that the speed of surface temperature convergence depends on factors such as the quality of initial boundary conditions, thermal inertia, ill…

2018 Monthly Notices of the Royal Astronomical Society
Rosetta 4
BEANS - a software package for distributed Big Data analysis
DOI: 10.1093/mnras/sty803 Bibcode: 2018MNRAS.477.3076H

Hypki, Arkadiusz

BEANS software is a web-based, easy to install and maintain, new tool to store and analyse in a distributed way a massive amount of data. It provides a clear interface for querying, filtering, aggregating, and plotting data from an arbitrary number of data sets. Its main purpose is to simplify the process of storing, examining, and finding new rel…

2018 Monthly Notices of the Royal Astronomical Society
Gaia 4
On the inner disc structure of MWC480: evidence for asymmetries?
DOI: 10.1093/mnras/stx2533 Bibcode: 2018MNRAS.473.3147J

Matter, A.; Lopez, B.; Sitko, M. L. +7 more

Studying the physical conditions structuring the young circumstellar discs is required for understanding the onset of planet formation. Of particular interest is the protoplanetary disc surrounding the Herbig star MWC480. The structure and properties of the circumstellar disc of MWC480 are studied by infrared interferometry and interpreted from a …

2018 Monthly Notices of the Royal Astronomical Society
ISO 4