Search Publications

A catalogue of Galactic supernova remnants in the far-infrared: revealing ejecta dust in pulsar wind nebulae
DOI: 10.1093/mnras/sty2942 Bibcode: 2019MNRAS.483...70C

De Looze, I.; Rho, J.; Dunne, L. +7 more

We search for far-infrared counterparts of known supernova remnants (SNRs) in the Galactic plane (10° < |l| < 60°) at 70-500 µm using the Herschel Infrared Galactic Plane Survey (Hi-GAL). Of 71 sources studied, we find that 29 (41 per cent) SNRs have a clear FIR detection of dust emission associated with the SNR. Dust from 8 of these i…

2019 Monthly Notices of the Royal Astronomical Society
Herschel 37
Homogeneously derived transit timings for 17 exoplanets and reassessed TTV trends for WASP-12 and WASP-4
DOI: 10.1093/mnras/stz2620 Bibcode: 2019MNRAS.490.1294B

Molina, D.; Bretton, M.; Jones, H. R. A. +34 more

We homogeneously analyse ∼3.2 × 105 photometric measurements for ∼1100 transit light curves belonging to 17 exoplanet hosts. The photometric data cover 16 years (2004-2019) and include amateur and professional observations. Old archival light curves were reprocessed using up-to-date exoplanetary parameters and empirically debiased limb-…

2019 Monthly Notices of the Royal Astronomical Society
Gaia eHST 37
Constraining the evolution of stellar rotation using solar twins
DOI: 10.1093/mnrasl/slz034 Bibcode: 2019MNRAS.485L..68L

Bedell, Megan; Meléndez, Jorge; Bean, Jacob L. +7 more

The stellar rotation versus age relation is commonly considered a useful tool to derive reliable ages for Sun-like stars. However, in the light of Kepler data, the presence of apparently old and fast rotators that do not obey the usual gyrochronology relations led to the hypothesis of weakened magnetic breaking in some stars. In this letter, we co…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 37
Searching for the GD-1 stream progenitor in Gaia DR2 with direct N-body simulations
DOI: 10.1093/mnras/stz867 Bibcode: 2019MNRAS.485.5929W

Bovy, Jo; Webb, Jeremy J.

We perform a large suite of direct N-body simulations aimed at revealing the location of the progenitor, or its remnant, of the GD-1 stream. Data from Gaia DR2 reveal that the GD-1 stream extends over ≈100°, allowing us to determine the stream's leading and trailing ends. Our models suggest that the length of the stream is consistent with a dynami…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 37
The magnetic early B-type Stars II: stellar atmospheric parameters in the era of Gaia
DOI: 10.1093/mnras/stz416 Bibcode: 2019MNRAS.485.1508S

Wade, G. A.; Neiner, C.; Shultz, M. E. +6 more

Atmospheric parameters determined via spectral modelling are unavailable for many of the known magnetic early B-type stars. We utilized high-resolution spectra together with non-local thermodynamic equilibrium models to measure effective temperatures Teff and surface gravities log g of stars for which these measurements are not yet avai…

2019 Monthly Notices of the Royal Astronomical Society
Gaia Hipparcos 37
Brown dwarf census with the Dark Energy Survey year 3 data and the thin disc scale height of early L types
DOI: 10.1093/mnras/stz2398 Bibcode: 2019MNRAS.489.5301C

Bechtol, K.; Smith, M.; Abbott, T. M. C. +46 more

In this paper we present a catalogue of 11 745 brown dwarfs with spectral types ranging from L0 to T9, photometrically classified using data from the Dark Energy Survey (DES) year 3 release matched to the Vista Hemisphere Survey (VHS) DR3 and Wide-field Infrared Survey Explorer (WISE) data, covering ≈2400 deg2 up to iAB = 22.…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 37
Strong lensing reveals jets in a sub-microJy radio-quiet quasar
DOI: 10.1093/mnras/stz510 Bibcode: 2019MNRAS.485.3009H

Jackson, N.; Sluse, D.; Stacey, H. R. +2 more

We present e-MERLIN and European VLBI Network observations which reveal unambiguous jet activity within radio-quiet quasar HS 0810+2554. With an intrinsic flux density of 880 nJy, this is the faintest radio source ever imaged. The findings present new evidence against the idea that radio-loud and radio-quiet quasars are powered by different underl…

2019 Monthly Notices of the Royal Astronomical Society
eHST 37
The haloes and environments of nearby galaxies (HERON) - I. Imaging, sample characteristics, and envelope diameters
DOI: 10.1093/mnras/stz2106 Bibcode: 2019MNRAS.490.1539R

Sales, Laura; Kormendy, John; Rich, R. Michael +16 more

We use a dedicated 0.7-m telescope to image the haloes of 119 galaxies in the Local Volume to µr ∼ 28-30 mag arcsec-2. The sample is primarily from the Two Micron All Sky Survey Large Galaxy Atlas (Jarrett et al. 2003) and extended to include nearby dwarf galaxies and more distant giant ellipticals, and spans fully the …

2019 Monthly Notices of the Royal Astronomical Society
Gaia 37
The VISCACHA survey - I. Overview and first results
DOI: 10.1093/mnras/stz369 Bibcode: 2019MNRAS.484.5702M

Piatti, Andrés E.; Barbuy, Beatriz; Bica, Eduardo +15 more

The VISCACHA (VIsible Soar photometry of star Clusters in tApii and Coxi HuguA) Survey is an ongoing project based on deep photometric observations of Magellanic Cloud star clusters, collected using the SOuthern Astrophysical Research (SOAR) telescope together with the SOAR Adaptive Module Imager. Since 2015 more than 200 h of telescope time were …

2019 Monthly Notices of the Royal Astronomical Society
Gaia 37
Evidence for an emerging disc wind and collimated outflow during an X-ray flare in the narrow-line Seyfert 1 galaxy Mrk 335
DOI: 10.1093/mnras/stz274 Bibcode: 2019MNRAS.484.4287G

Kriss, G. A.; Fabian, A. C.; Pinto, C. +13 more

A triggered 140{ ks}XMM-Newton observation of the narrow-line Seyfert 1 (NLS1) Mrk 335 in 2015 December caught the active galaxy at its lowest X-ray flux since 2007. The NLS1 is relatively quiescent for the first {∼ }120{ ks} of the observation before it flares in brightness by a factor of about five in the last 20{ ks}. Although only part of the …

2019 Monthly Notices of the Royal Astronomical Society
XMM-Newton 37