Search Publications

Calibration of Herschel SPIRE FTS observations at different spectral resolutions
DOI: 10.1093/mnras/stw2600 Bibcode: 2017MNRAS.464.3331M

Valtchanov, I.; Hopwood, R.; Spencer, L. +11 more

The SPIRE Fourier Transform Spectrometer on-board the Herschel Space Observatory had two standard spectral resolution modes for science observations: high resolution (HR) and low resolution (LR), which could also be performed in sequence (H+LR). A comparison of the HR and LR resolution spectra taken in this sequential mode revealed a systematic di…

2017 Monthly Notices of the Royal Astronomical Society
Herschel 3
Superwind evolution: the young starburst-driven wind galaxy NGC 2782
DOI: 10.1093/mnras/stx327 Bibcode: 2017MNRAS.467.3788B

Stevens, Ian R.; Bravo-Guerrero, Jimena

We present results from a 30-ks Chandra observation of the important starburst galaxy NGC 2782, covering the 0.3-10 keV energy band. We find evidence of a superwind of small extent, which is likely in an early stage of development. We find a total of 27 X-ray point sources within a region of radius 2D25 of the galaxy centre and that are…

2017 Monthly Notices of the Royal Astronomical Society
eHST 3
Dust scattering from the Taurus Molecular Cloud
DOI: 10.1093/mnras/stw3280 Bibcode: 2017MNRAS.466.3199N

Murthy, Jayant; Narayan, Sathya; Karuppath, Narayanankutty

We present an analysis of the diffuse ultraviolet emission near the Taurus Molecular Cloud based on observations made by the Galaxy Evolution Explorer. We used a Monte Carlo dust scattering model to show that about half of the scattered flux originates in the molecular cloud with 25 per cent arising in the foreground and 25 per cent behind the clo…

2017 Monthly Notices of the Royal Astronomical Society
Planck 3
Hubble Space Telescope observations of BALQSO Ton 34 reveal a connection between the broad-line region and the BAL outflow
DOI: 10.1093/mnras/stx669 Bibcode: 2017MNRAS.468.3607K

Binette, L.; Bianchi, L.; Nicastro, F. +7 more

Ton 34 recently transitioned from non-absorbing quasar into a broad absorption line quasi-stellar object. Here, we report new HST-STIS observations of this quasar. Along with C IV absorption, we also detect absorption by NV+Lyα and possibly O VI+Lyβ. We follow the evolution of the C IV BAL, and find that, for the slower outflowing material, the ab…

2017 Monthly Notices of the Royal Astronomical Society
eHST 3
Local two-sample testing: a new tool for analysing high-dimensional astronomical data
DOI: 10.1093/mnras/stx1807 Bibcode: 2017MNRAS.471.3273F

Freeman, P. E.; Kim, I.; Lee, A. B.

Modern surveys have provided the astronomical community with a flood of high-dimensional data, but analyses of these data often occur after their projection to lower dimensional spaces. In this work, we introduce a local two-sample hypothesis test framework that an analyst may directly apply to data in their native space. In this framework, the an…

2017 Monthly Notices of the Royal Astronomical Society
eHST 2
On the signatures of flare-induced global waves in the Sun: GOLF and VIRGO observations
DOI: 10.1093/mnras/stx1953 Bibcode: 2017MNRAS.471.4677K

García, Rafael A.; Kumar, Brajesh; Mathur, Savita +1 more

Recently, several efforts have been made to identify the seismic signatures of flares and magnetic activity in the Sun and Sun-like stars. In this work, we have analysed the disc-integrated velocity and intensity observations of the Sun obtained from the Global Oscillations at Low Frequencies (GOLF) and Variability of solar IRradiance and Gravity …

2017 Monthly Notices of the Royal Astronomical Society
SOHO 2
Application of beam deconvolution technique to power spectrum estimation for CMB measurements
DOI: 10.1093/mnras/stw3122 Bibcode: 2017MNRAS.466.1348K

Keihänen, E.; Kurki-Suonio, H.; Reinecke, M. +1 more

We present two novel methods for the estimation of the angular power spectrum of cosmic microwave background (CMB) anisotropies. We assume an absolute CMB experiment with arbitrary asymmetric beams and arbitrary sky coverage. The methods differ from the earlier ones in that the power spectrum is estimated directly from the time-ordered data, witho…

2017 Monthly Notices of the Royal Astronomical Society
Planck 2
The highly ionized, high-velocity gas in NGC 6231
DOI: 10.1093/mnras/stw2762 Bibcode: 2017MNRAS.465.1023M

Massa, Derck

It is well known that clusters of massive stars are influenced by the presence of strong winds, that they are sources of diffuse X-rays from shocked gas, and that this gas can be vented into the surrounding region or the halo through the champagne effect. However, the details of how these different environments interact and evolve are far from com…

2017 Monthly Notices of the Royal Astronomical Society
IUE eHST 2
A three-dimensional orbit for the binary star Alpha Andromedae
DOI: 10.1093/mnras/stw2393 Bibcode: 2017MNRAS.464.1095B

Branham, Richard L., Jr.

Stars that are both spectroscopic and optical binaries present a means to determine simultaneously the masses of the components and the distance of the system independent of trigonometric parallax. Alpha Andromedae (Alpheratz) represents such a system and, moreover, the primary is the brightest of the mercury-manganese stars. An orbit, based on 42…

2017 Monthly Notices of the Royal Astronomical Society
Hipparcos 2
Detection of helicoidal motion in the optical jet of PKS 0521-365
DOI: 10.1093/mnrasl/slx090 Bibcode: 2017MNRAS.470L.107J

Jiménez-Andrade, E. F.; Falomo, R.; Chavushyan, V. +5 more

The jet activity of active galactic nuclei (AGNs), and its interaction with the interstellar medium, may play a pivotal role in the processes that regulate the growth and star formation of its host galaxy. Observational evidence that pinpoints the conditions of such interaction is paramount to unveil the physical processes involved. We report on t…

2017 Monthly Notices of the Royal Astronomical Society
eHST 2