Search Publications

Observation of variable pre-eclipse dips and disc windsin the eclipsing LMXB XTE J1710-281
DOI: 10.1093/mnras/sty918 Bibcode: 2018MNRAS.477.5358R

Maitra, Chandreyee; Paul, Biswajit; Raman, Gayathri

We report the first detection of highly ionized Fe species in the X-ray spectrum of the eclipsing and dipping Low-Mass X-ray Binary XTE J1710-281. Using archival Chandra and Suzaku observations, we have carried out a spectro-timing analysis of the source during three different epochs. We compare the average orbital profile and obtain differences i…

2018 Monthly Notices of the Royal Astronomical Society
Suzaku 12
Synchronized observations of bright points from the solar photosphere to the corona
DOI: 10.1093/mnras/sty020 Bibcode: 2018MNRAS.476..868T

Tavabi, Ehsan

One of the most important features in the solar atmosphere is the magnetic network and its relationship to the transition region (TR) and coronal brightness. It is important to understand how energy is transported into the corona and how it travels along the magnetic field lines between the deep photosphere and chromosphere through the TR and coro…

2018 Monthly Notices of the Royal Astronomical Society
IRIS 12
LBT/MODS spectroscopy of globular clusters in the irregular galaxy NGC 4449
DOI: 10.1093/mnras/sty344 Bibcode: 2018MNRAS.476.1942A

Tosi, M.; Cusano, F.; Mignoli, M. +10 more

We present intermediate-resolution (R ∼ 1000) spectra in the ∼3500-10 000 Å range of 14 globular clusters in the Magellanic irregular galaxy NGC 4449 acquired with the Multi-Object Double Spectrograph on the Large Binocular Telescope. We derived Lick indices in the optical and the Ca II triplet index in the near-infrared in order to infer the clus…

2018 Monthly Notices of the Royal Astronomical Society
eHST 12
K2 observations of the rapidly oscillating Ap star 33 Lib (HD 137949): new frequencies and unique non-linear interactions
DOI: 10.1093/mnras/sty2053 Bibcode: 2018MNRAS.480.2976H

Bowman, D. M.; Kurtz, D. W.; Cunha, M. S. +2 more

We present the analysis of K2 short cadence data of the rapidly oscillating Ap (roAp) star, 33 Librae (HD 137949). The precision afforded to the K2 data allow us to identify at least 11 pulsation modes in this star, compared to the three previously reported. Reoccurring separations between these modes lead us to suggest a large frequency separatio…

2018 Monthly Notices of the Royal Astronomical Society
Gaia 12
A distant sample of halo wide binaries from SDSS
DOI: 10.1093/mnras/sty2141 Bibcode: 2018MNRAS.480.4302C

Gould, Andrew; Coronado, Johanna; Chanamé, Julio +1 more

Samples of reliably identified halo wide binaries are scarce. If reasonably free from selection effects and with a small degree of contamination by chance alignments, these wide binaries become a powerful dynamical tool, having provided one of the very few experiments capable of constraining the nature of dark matter in the Milky Way halo. Current…

2018 Monthly Notices of the Royal Astronomical Society
Gaia 12
Agnostic stacking of intergalactic doublet absorption: measuring the Ne VIII population
DOI: 10.1093/mnras/sty294 Bibcode: 2018MNRAS.476.1356F

Shull, J. Michael; Danforth, Charles W.; Mathur, Smita +2 more

We present a blind search for doublet intergalactic metal absorption with a method dubbed `agnostic stacking'. Using a forward-modelling framework, we combine this with direct detections in the literature to measure the overall metal population. We apply this novel approach to the search for Ne VIII absorption in a set of 26 high-quality COS spect…

2018 Monthly Notices of the Royal Astronomical Society
eHST 12
Establishing the spectral turnover of blazar PKS 2155-304 as an outcome of radiative losses
DOI: 10.1093/mnrasl/sly086 Bibcode: 2018MNRAS.478L.105J

Jeena, K.; Misra, R.; Ravikumar, C. D. +2 more

The broad-band optical/UV and X-ray spectra of blazars have been often modelled as synchrotron component arising from a broken power-law distribution of electrons. A broken power-law distribution is expected, since the high-energy electrons undergo radiative losses effectively. The change in the energy index should then be ≈1 and corresponds to a …

2018 Monthly Notices of the Royal Astronomical Society
XMM-Newton 11
On the nature of the high-energy rollover in 1H 0419-577
DOI: 10.1093/mnras/sty318 Bibcode: 2018MNRAS.476.1258T

Turner, T. J.; Reeves, J. N.; Braito, V. +1 more

A NuSTAR/Swift observation of the luminous Seyfert 1 galaxy 1H 0419-577 taken during 2015 reveals one of the most extreme high-energy cut-offs observed to date from an AGN - an origin due to thermal Comptonization would imply a remarkably low coronal temperature kT ∼ 15 keV. The low-energy peak of the spectrum in the hard X-ray NuSTAR band, which …

2018 Monthly Notices of the Royal Astronomical Society
XMM-Newton 11
Quantifying the abundance of faint, low-redshift satellite galaxies in the COSMOS survey
DOI: 10.1093/mnras/sty1333 Bibcode: 2018MNRAS.478.5336X

Rhodes, Jason; Taylor, James E.; Koekemoer, Anton +3 more

Faint dwarf satellite galaxies are important as tracers of small-scale structure, but remain poorly characterized outside the Local Group, due to the difficulty of identifying them consistently at larger distances. We review a recently proposed method for estimating the average satellite population around a given sample of nearby bright galaxies, …

2018 Monthly Notices of the Royal Astronomical Society
eHST 11
Positron annihilation in the nuclear outflows of the Milky Way
DOI: 10.1093/mnrasl/slx183 Bibcode: 2018MNRAS.474L..17P

Ruiter, Ashley J.; Panther, Fiona H.; Seitenzahl, Ivo R. +2 more

Observations of soft gamma rays emanating from the Milky Way from SPI/INTEGRAL reveal the annihilation of ∼2 × 1043 positrons every second in the Galactic bulge. The origin of these positrons, which annihilate to produce a prominent emission line centred at 511 keV, has remained mysterious since their discovery almost 50 yr ago. A plaus…

2018 Monthly Notices of the Royal Astronomical Society
INTEGRAL 11