Search Publications

Eclipsing binary stars with a δ Scuti component
DOI: 10.1093/mnras/stx1241 Bibcode: 2017MNRAS.470..915K

Smalley, B.; Kahraman Aliçavuş, F.; Kubát, J. +1 more

Eclipsing binaries with a δ Sct component are powerful tools to derive the fundamental parameters and probe the internal structure of stars. In this study, spectral analysis of six primary δ Sct components in eclipsing binaries has been performed. Values of Teff, v sin I, and metallicity for the stars have been derived from medium-resol…

2017 Monthly Notices of the Royal Astronomical Society
Gaia 59
The most distant, luminous, dusty star-forming galaxies: redshifts from NOEMA and ALMA spectral scans
DOI: 10.1093/mnras/stx1956 Bibcode: 2017MNRAS.472.2028F

Pérez-Fournon, I.; Ivison, R. J.; Omont, A. +23 more

We present 1.3- and/or 3-mm continuum images and 3-mm spectral scans, obtained using Northern Extended Millimeter Array (NOEMA) and Atacama Large Millimeter Array (ALMA), of 21 distant, dusty, star-forming galaxies. Our sample is a subset of the galaxies selected by Ivison et al. on the basis of their extremely red far-infrared (far-IR) colours an…

2017 Monthly Notices of the Royal Astronomical Society
Herschel 59
A high fraction of Be stars in young massive clusters: evidence for a large population of near-critically rotating stars
DOI: 10.1093/mnras/stw3042 Bibcode: 2017MNRAS.465.4795B

Cabrera-Ziri, I.; Usher, C.; Bastian, N. +6 more

Recent photometric analyses of the colour-magnitude diagrams of young massive clusters (YMCs) have found evidence for splitting in the main sequence and extended main-sequence turn-offs, both of which have been suggested to be caused by stellar rotation. Comparison of the observed main-sequence splitting with models has led various authors to sugg…

2017 Monthly Notices of the Royal Astronomical Society
eHST 59
The statistical properties of neutral gas at z < 1.65 from UV measurements of Damped Lyman Alpha systems
DOI: 10.1093/mnras/stx1787 Bibcode: 2017MNRAS.471.3428R

Turnshek, David A.; Rao, Sandhya M.; Monier, Eric M. +1 more

We derive the statistical properties of neutral gas at redshifts 0.11 < z < 1.65 from ultraviolet (UV) measurements of quasar Ly α absorption lines corresponding to 369 Mg II systems with W^{λ 2796}0 ≥ 0.3 Å. In addition to the 41 damped Lyman alpha (DLA) systems presented in Rao et al. (2006), the current DLA sample includes 29 n…

2017 Monthly Notices of the Royal Astronomical Society
eHST 59
Intergalactic Lyman continuum photon budget in the past 5 billion years
DOI: 10.1093/mnras/stw3086 Bibcode: 2017MNRAS.466..838G

Khaire, Vikram; Srianand, Raghunathan; Choudhury, Tirthankar Roy +1 more

We constrain the H I photoionization rate (Γ _{H I}) at z ≲ 0.45 by comparing the flux probability distribution function and power spectrum of the Lyα forest data along 82 Quasi-Stellar Object (QSO) sightlines obtained using Cosmic Origins Spectrograph with models generated from smoothed particle hydrodynamic simulations. We have developed a modul…

2017 Monthly Notices of the Royal Astronomical Society
eHST 58
Swift observations of V404 Cyg during the 2015 outburst: X-ray outflows from super-Eddington accretion
DOI: 10.1093/mnras/stx1699 Bibcode: 2017MNRAS.471.1797M

Altamirano, D.; Sanna, A.; Knigge, C. +11 more

The black hole (BH) binary V404 Cyg entered the outburst phase in 2015 June after 26 yr of X-ray quiescence, and with its behaviour broke the outburst evolution pattern typical of most BH binaries. We observed the entire outburst with the Swift satellite and performed time-resolved spectroscopy of its most active phase, obtaining over a thousand s…

2017 Monthly Notices of the Royal Astronomical Society
INTEGRAL 58
Interpreting the star formation efficiency of nearby molecular clouds with ionizing radiation
DOI: 10.1093/mnras/stx1765 Bibcode: 2017MNRAS.471.4844G

Hennebelle, Patrick; Soler, Juan D.; Geen, Sam

We investigate the origin of observed local star formation relations using radiative magnetohydrodynamic simulations with self-consistent star formation and ionizing radiation. We compare these clouds to the density distributions of local star-forming clouds and find that the most diffuse simulated clouds match the observed clouds relatively well.…

2017 Monthly Notices of the Royal Astronomical Society
Planck 57
Close entrainment of massive molecular gas flows by radio bubbles in the central galaxy of Abell 1795
DOI: 10.1093/mnras/stx2255 Bibcode: 2017MNRAS.472.4024R

Fabian, A. C.; Combes, F.; McDonald, M. +8 more

We present new ALMA observations tracing the morphology and velocity structure of the molecular gas in the central galaxy of the cluster Abell 1795. The molecular gas lies in two filaments that extend 5-7 kpc to the N and S from the nucleus and project exclusively around the outer edges of two inner radio bubbles. Radio jets launched by the centra…

2017 Monthly Notices of the Royal Astronomical Society
eHST 57
The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements from DR12 galaxy clustering - towards an accurate model
DOI: 10.1093/mnras/stx1641 Bibcode: 2017MNRAS.471.2370C

Rubiño-Martín, J. A.; Brownstein, Joel R.; Ho, Shirley +28 more

We analyse the broad-range shape of the monopole and quadrupole correlation functions of the Baryon Oscillation Spectroscopic Survey Data Release 12 (DR12) CMASS and LOWZ galaxy sample to obtain constraints on the Hubble expansion rate H(z), the angular-diameter distance DA(z), the normalized growth rate f(z)σ8(z) and the phy…

2017 Monthly Notices of the Royal Astronomical Society
Planck 57
The X-ray properties of Be/X-ray pulsars in quiescence
DOI: 10.1093/mnras/stx1255 Bibcode: 2017MNRAS.470..126T

Tsygankov, Sergey S.; Lutovinov, Alexander A.; Poutanen, Juri +2 more

Observations of accreting neutron stars (NSs) with strong magnetic fields can be used not only for studying the accretion flow interaction with the NS magnetospheres, but also for understanding the physical processes inside NSs and for estimating their fundamental parameters. Of particular interest are (I) the interaction of a rotating NS (magneto…

2017 Monthly Notices of the Royal Astronomical Society
XMM-Newton 57