Search Publications

Star formation complexes in the `galaxy-sized' supergiant shell of the galaxy HolmbergI
DOI: 10.1093/mnras/sty1158 Bibcode: 2018MNRAS.478.3386E

Egorov, Oleg V.; Lozinskaya, Tatiana A.; Moiseev, Alexei V. +1 more

We present the results of observations of the galaxy Holmberg I carried out at the Russian 6-m telescope in the narrow-band imaging, long-slit spectroscopy, and scanning Fabry-Perot interferometer modes. A detailed analysis of gas kinematics, ionization conditions, and metallicity of star-forming regions in the galaxy is presented. The aim of the …

2018 Monthly Notices of the Royal Astronomical Society
eHST 28
Cometary plasma response to interplanetary corotating interaction regions during 2016 June-September: a quantitative study by the Rosetta Plasma Consortium
DOI: 10.1093/mnras/sty2166 Bibcode: 2018MNRAS.480.4544H

Henri, Pierre; Simon Wedlund, Cyril; Nilsson, Hans +14 more

Four interplanetary corotating interaction regions (CIRs) were identified during 2016 June-September by the Rosetta Plasma Consortium (RPC) monitoring in situ the plasma environment of the comet 67P/Churyumov-Gerasimenko (67P) at heliocentric distances of ∼3-3.8 au. The CIRs, formed in the interface region between low- and high-speed solar wind st…

2018 Monthly Notices of the Royal Astronomical Society
Rosetta 28
Mass-invariance of the iron enrichment in the hot haloes of massive ellipticals, groups, and clusters of galaxies
DOI: 10.1093/mnrasl/sly080 Bibcode: 2018MNRAS.478L.116M

Urdampilleta, I.; Simionescu, A.; Kaastra, J. S. +7 more

X-ray measurements find systematically lower Fe abundances in the X-ray emitting haloes pervading groups (kT ≲ 1.7 keV) than in clusters of galaxies. These results have been difficult to reconcile with theoretical predictions. However, models using incomplete atomic data or the assumption of isothermal plasmas may have biased the best-fitting Fe a…

2018 Monthly Notices of the Royal Astronomical Society
XMM-Newton 28
Ground-based detection of G star superflares with NGTS
DOI: 10.1093/mnras/sty897 Bibcode: 2018MNRAS.477.4655J

Jackman, James A. G.; Wheatley, Peter J.; Günther, Maximilian N. +19 more

We present high cadence detections of two superflares from a bright G8 star (V = 11.56) with the Next Generation Transit Survey (NGTS). We improve upon previous superflare detections by resolving the flare rise and peak, allowing us to fit a solar flare inspired model without the need for arbitrary break points between rise and decay. Our data als…

2018 Monthly Notices of the Royal Astronomical Society
Gaia 28
SDSS J211852.96-073227.5: a new γ-ray flaring narrow-line Seyfert 1 galaxy
DOI: 10.1093/mnras/sty904 Bibcode: 2018MNRAS.477.5127Y

Komossa, S.; Yang, Hui; Jin, Chichuan +6 more

We report on the identification of a new γ-ray-emitting narrow-line Seyfert 1 (NLS1) galaxy, SDSS J211852.96-073227.5 (hereinafter J2118-0732). The galaxy, at a redshift of 0.26, is associated with a radio source of flat/inverted spectrum at high radio frequencies. The analysis of its optical spectrum obtained in the Sloan Digital Sky Survey (SDSS…

2018 Monthly Notices of the Royal Astronomical Society
XMM-Newton 28
Galactic outflows, star formation histories, and time-scales in starburst dwarf galaxies from STARBIRDS
DOI: 10.1093/mnras/sty839 Bibcode: 2018MNRAS.477.3164M

McQuinn, Kristen B. W.; Skillman, Evan D.; Kelley, Tyler +2 more

Winds are predicted to be ubiquitous in low-mass, actively star-forming galaxies. Observationally, winds have been detected in relatively few local dwarf galaxies, with even fewer constraints placed on their time-scales. Here, we compare galactic outflows traced by diffuse, soft X-ray emission from Chandra Space Telescope archival observations to …

2018 Monthly Notices of the Royal Astronomical Society
eHST 28
Stellar ages and masses in the solar neighbourhood: Bayesian analysis using spectroscopy and Gaia DR1 parallaxes
DOI: 10.1093/mnras/sty709 Bibcode: 2018MNRAS.477.2966L

Ting, Yuan-Sen; Dotter, Aaron; Lin, Jane +1 more

We present a Bayesian implementation of isochrone fitting in deriving stellar ages and masses, incorporating absolute K magnitude (M_K) derived from 2MASS photometry and Gaia DR1 parallax and differentiation between initial bulk metallicity and present-day surface metallicity, with allowance for incorporating further constraints (e.g. asteroseismo…

2018 Monthly Notices of the Royal Astronomical Society
Gaia Hipparcos 28
KiDS-i-800: comparing weak gravitational lensing measurements from same-sky surveys
DOI: 10.1093/mnras/sty859 Bibcode: 2018MNRAS.477.4285A

Heymans, C.; Wolf, C.; Lidman, C. +21 more

We present a weak gravitational lensing analysis of 815 deg2 of i-band imaging from the Kilo-Degree Survey (KiDS-i-800). In contrast to the deep r-band observations, which take priority during excellent seeing conditions and form the primary KiDS data set (KiDS-r-450), the complementary yet shallower KiDS-i-800 spans a wide range of obs…

2018 Monthly Notices of the Royal Astronomical Society
Gaia 28
On the production of He, C, and N by low- and intermediate-mass stars: a comparison of observed and model-predicted planetary nebula abundances
DOI: 10.1093/mnras/stx2286 Bibcode: 2018MNRAS.473..241H

Balick, B.; Henry, R. B. C.; Stephenson, B. G. +2 more

The primary goal of this paper is to make a direct comparison between the measured and model-predicted abundances of He, C, and N in a sample of 35 well-observed Galactic planetary nebulae (PNe). All observations, data reductions, and abundance determinations were performed in house to ensure maximum homogeneity. Progenitor star masses (M ≤ 4 M

2018 Monthly Notices of the Royal Astronomical Society
IUE eHST 28
Unmasking the hidden NGTS-3Ab: a hot Jupiter in an unresolved binary system
DOI: 10.1093/mnras/sty1193 Bibcode: 2018MNRAS.478.4720G

Smalley, Barry; Gibson, Neale P.; Wheatley, Peter J. +36 more

We present the discovery of NGTS-3Ab, a hot Jupiter found transiting the primary star of an unresolved binary system. We develop a joint analysis of multicolour photometry, centroids, radial velocity (RV) cross-correlation function (CCF) profiles, and their bisector inverse slopes (BIS) to disentangle this three-body system. Data from the Next Gen…

2018 Monthly Notices of the Royal Astronomical Society
Gaia 27