Search Publications

A new method for probing magnetic field strengths from striations in the interstellar medium
DOI: 10.1093/mnras/sty2677 Bibcode: 2018MNRAS.481.5275T

Federrath, Christoph; Tassis, Konstantinos; Schneider, Nicola +1 more

Recent studies of the diffuse parts of molecular clouds have revealed the presence of parallel, ordered low-density filaments termed striations. Flows along magnetic field lines, Kelvin-Helmholtz instabilities and hydromagnetic waves are amongst the various formation mechanisms proposed. Through a synergy of observational, numerical, and theoretic…

2018 Monthly Notices of the Royal Astronomical Society
Herschel 20
Cresting the wave: proper motions of the Eastern Banded Structure
DOI: 10.1093/mnras/stx2528 Bibcode: 2018MNRAS.473.2428D

Belokurov, Vasily; Koposov, Sergey E.; Deason, Alis J.

We study the kinematic properties of the Eastern Banded Structure (EBS) and Hydra I overdensity using exquisite proper motions derived from the Sloan Digital Sky Survey (SDSS) and Gaia source catalogue. Main sequence turn-off stars in the vicinity of the EBS are identified from SDSS photometry; we use the proper motions and, where applicable, spec…

2018 Monthly Notices of the Royal Astronomical Society
Gaia 20
Atmospheric stellar parameters for large surveys using FASMA, a new spectral synthesis package
DOI: 10.1093/mnras/stx2564 Bibcode: 2018MNRAS.473.5066T

Sousa, S. G.; Santos, N. C.; Bruzual, G. +4 more

In the era of vast spectroscopic surveys focusing on Galactic stellar populations, astronomers want to exploit the large quantity and good quality of data to derive their atmospheric parameters without losing precision from automatic procedures. In this work, we developed a new spectral package, FASMA, to estimate the stellar atmospheric parameter…

2018 Monthly Notices of the Royal Astronomical Society
Gaia 20
Signature of inverse Compton emission from blazars
DOI: 10.1093/mnras/stx2553 Bibcode: 2018MNRAS.473.3638G

Gaur, Haritma; Mohan, Prashanth; Wierzcholska, Alicja +1 more

Blazars are classified into high-, intermediate- and low-energy-peaked sources based on the location of their synchrotron peak. This lies in infra-red/optical to ultra-violet bands for low- and intermediate-peaked blazars. The transition from synchrotron to inverse Compton emission falls in the X-ray bands for such sources. We present the spectral…

2018 Monthly Notices of the Royal Astronomical Society
XMM-Newton 20
Multiplicity of disc-bearing stars in Upper Scorpius and Upper Centaurus-Lupus
DOI: 10.1093/mnras/sty2108 Bibcode: 2018MNRAS.480.5099K

Federrath, Christoph; Bento, Joao; Ireland, Michael +2 more

We present observations of disc-bearing stars in Upper Scorpius (US) and Upper Centaurus-Lupus (UCL) with moderate resolution spectroscopy in order to determine the influence of multiplicity on disc persistence after ∼ 5-20 Myr. Discs were identified using infrared (IR) excess from the Wide-field Infrared Survey Explorer (WISE) survey. Our survey …

2018 Monthly Notices of the Royal Astronomical Society
Gaia 20
The Carnegie RR Lyrae Program: mid-infrared period-luminosity relations of RR Lyrae stars in Reticulum
DOI: 10.1093/mnras/sty1959 Bibcode: 2018MNRAS.480.4138M

Madore, Barry F.; Freedman, Wendy L.; Scowcroft, Victoria +4 more

We analysed 30 RR Lyrae stars (RRLs) located in the Large Magellanic Cloud (LMC) globular cluster Reticulum that were observed in the 3.6 and 4.5 µ m passbands with the Infrared Array Camera (IRAC) on board the Spitzer Space Telescope. We derived new mid-infrared (MIR) period-luminosity (PL) relations. The zero points of the PL relations wer…

2018 Monthly Notices of the Royal Astronomical Society
Gaia 20
The shape of galaxy dark matter haloes in massive galaxy clusters: insights from strong gravitational lensing
DOI: 10.1093/mnras/sty909 Bibcode: 2018MNRAS.477.4046J

Massey, Richard; Jauzac, Mathilde; Harvey, David

We assess how much unused strong lensing information is available in the deep Hubble Space Telescope imaging and Very Large Telescope/Multi Unit Spectroscopic Explorer spectroscopy of the Frontier Field clusters. As a pilot study, we analyse galaxy cluster MACS J0416.1-2403 (z = 0.397, M(R < 200 kpc) = 1.6 × 1014 M), whic…

2018 Monthly Notices of the Royal Astronomical Society
eHST 20
Alone on a wide wide sea. The origin of SECCO 1, an isolated star-forming gas cloud in the Virgo cluster*†‡
DOI: 10.1093/mnras/sty467 Bibcode: 2018MNRAS.476.4565B

Bellazzini, M.; Testa, V.; Beccari, G. +12 more

SECCO 1 is an extremely dark, low-mass (M ≃ 105 M), star-forming stellar system lying in the low-velocity cloud (LVC) substructure of the Virgo cluster of galaxies, and hosting several H II regions. Here, we review our knowledge of this remarkable system, and present the results of (a) additional analysis of our …

2018 Monthly Notices of the Royal Astronomical Society
eHST 20
The PHEMU15 catalogue and astrometric results of the Jupiter's Galilean satellite mutual occultation and eclipse observations made in 2014-2015
DOI: 10.1093/mnras/stx2957 Bibcode: 2018MNRAS.474.4730S

Delcroix, M.; Colas, F.; Carry, B. +116 more

During the 2014-2015 mutual events season, the Institut de Mécanique Céleste et de Calcul des Éphémérides (IMCCE), Paris, France, and the Sternberg Astronomical Institute (SAI), Moscow, Russia, led an international observation campaign to record ground-based photometric observations of Galilean moon mutual occultations and eclipses. We focused on …

2018 Monthly Notices of the Royal Astronomical Society
Gaia 20
Unbiased TGAS×LAMOST distances and the role of binarity
DOI: 10.1093/mnras/sty2468 Bibcode: 2018MNRAS.481.2970C

Rix, Hans-Walter; Coronado, Johanna; Trick, Wilma H.

Spectrophotometric distances to stars observed by large spectroscopic surveys offer a crucial complement to parallax distances that remain very important also after the future Gaia data releases. Here, we present a probabilistic approach to modelling spectroscopic information for a subset of 4000 main sequence stars with good parallaxes (σϖ

2018 Monthly Notices of the Royal Astronomical Society
Gaia 20