Search Publications

Probing the cool interstellar and circumgalactic gas of three massive lensing galaxies at z = 0.4-0.7
DOI: 10.1093/mnras/stw484 Bibcode: 2016MNRAS.458.2423Z

Zahedy, Fakhri S.; Chen, Hsiao-Wen; Rauch, Michael +2 more

We present multisightline absorption spectroscopy of cool gas around three lensing galaxies at z = 0.4-0.7. These lenses have half-light radii re = 2.6-8 kpc and stellar masses of log M*/M = 10.9-11.4, and therefore resemble nearby passive elliptical galaxies. The lensed QSO sightlines presented here occur at proj…

2016 Monthly Notices of the Royal Astronomical Society
eHST 58
Acceleration of individual, decimetre-sized aggregates in the lower coma of comet 67P/Churyumov-Gerasimenko
DOI: 10.1093/mnras/stw2179 Bibcode: 2016MNRAS.462S..78A

Jorda, L.; Lamy, P. L.; Lara, L. M. +41 more

We present observations of decimetre-sized, likely ice-containing aggregates ejected from a confined region on the surface of comet 67P/Churyumov-Gerasimenko. The images were obtained with the narrow angle camera of the Optical, Spectroscopic, and Infrared Remote Imaging System on board the Rosetta spacecraft in 2016 January when the comet was at …

2016 Monthly Notices of the Royal Astronomical Society
Rosetta 57
The SCUBA-2 Cosmology Legacy Survey: galaxies in the deep 850 µm survey, and the star-forming `main sequence'
DOI: 10.1093/mnras/stw564 Bibcode: 2016MNRAS.458.4321K

Bowler, R. A. A.; McLure, R. J.; Dunlop, J. S. +14 more

We investigate the properties of the galaxies selected from the deepest 850-µm survey undertaken to date with (Submillimetre Common-User Bolometer Array 2) SCUBA-2 on the James Clerk Maxwell Telescope as part of the SCUBA-2 Cosmology Legacy Survey. A total of 106 sources (>5σ) were uncovered at 850 µm from an area of ≃150 arcmin

2016 Monthly Notices of the Royal Astronomical Society
Herschel eHST 56
A robust measurement of the mass outflow rate of the galactic outflow from NGC 6090
DOI: 10.1093/mnras/stw1951 Bibcode: 2016MNRAS.463..541C

Chisholm, John; Leitherer, Claus; Tremonti Christy, A. +1 more

To evaluate the impact of stellar feedback, it is critical to estimate the mass outflow rates of galaxies. Past estimates have been plagued by uncertain assumptions about the outflow geometry, metallicity, and ionization fraction. Here we use Hubble Space Telescope ultraviolet spectroscopic observations of the nearby starburst NGC 6090 to demonstr…

2016 Monthly Notices of the Royal Astronomical Society
eHST 56
Cosmochemical implications of CONSERT permittivity characterization of 67P/CG
DOI: 10.1093/mnras/stx040 Bibcode: 2016MNRAS.462S.516H

Lasue, J.; Quirico, E.; Kofman, W. +7 more

Analysis of the propagation of the Comet Nucleus Sounding Experiment by Radiowave Transmission (CONSERT) signal throughout the small lobe of the 67P/CG nucleus has permitted us to deduce the real part of the permittivity, at a value of 1.27 ± 0.05. The first interpretation of this value, using the dielectric properties of mixtures of ices (H2…

2016 Monthly Notices of the Royal Astronomical Society
Rosetta 55
A PSF-based approach to Kepler/K2 data - I. Variability within the K2 Campaign 0 star clusters M 35 and NGC 2158
DOI: 10.1093/mnras/stv2628 Bibcode: 2016MNRAS.456.1137L

Bedin, L. R.; Piotto, G.; Nardiello, D. +1 more

Kepler and K2 data analysis reported in the literature is mostly based on aperture photometry. Because of Kepler's large, undersampled pixels and the presence of nearby sources, aperture photometry is not always the ideal way to obtain high-precision photometry, and, because of this, the data set has not been fully exploited so far. We present a n…

2016 Monthly Notices of the Royal Astronomical Society
eHST 55
A Herschel-SPIRE survey of the Mon R2 giant molecular cloud: analysis of the gas column density probability density function
DOI: 10.1093/mnras/stw1303 Bibcode: 2016MNRAS.461...22P

Henning, T.; Gutermuth, R.; Wolk, S. J. +8 more

We present a far-IR survey of the entire Mon R2 giant molecular cloud (GMC) with Herschel-Spectral and Photometric Imaging REceiver cross-calibrated with Planck-High Frequency Instrument data. We fit the spectral energy distributions of each pixel with a greybody function and an optimal beta value of 1.8. We find that mid-range column densities ob…

2016 Monthly Notices of the Royal Astronomical Society
Herschel Planck 55
A young cluster with an extended main-sequence turnoff: confirmation of a prediction of the stellar rotation scenario
DOI: 10.1093/mnrasl/slw067 Bibcode: 2016MNRAS.460L..20B

Salaris, M.; Larsen, S.; Cabrera-Ziri, I. +13 more

We present Hubble Space Telescope photometry of NGC 1850, a ∼100 Myr, ∼105 M cluster in the Large Magellanic Cloud. The colour-magnitude diagram clearly shows the presence of an extended main-sequence turnoff (eMSTO). The use of non-rotating stellar isochrones leads to an age spread of ∼40 Myr. This is in good agreement with…

2016 Monthly Notices of the Royal Astronomical Society
eHST 54
Matching dust emission structures and magnetic field in high-latitude cloud L1642: comparing Herschel and Planck maps
DOI: 10.1093/mnras/stw1061 Bibcode: 2016MNRAS.460.1934M

Juvela, M.; Montier, L.; Ristorcelli, I. +7 more

The nearby cloud L1642 is one of only two known very high latitude (|b| > 30 deg) clouds actively forming stars. It is a rare example of star formation in isolated conditions, and can reveal important details of star formation in general, e.g. of the effect of magnetic fields. We compare Herschel dust emission structures and magnetic field orie…

2016 Monthly Notices of the Royal Astronomical Society
Herschel Planck 54
SU Lyncis, a hard X-ray bright M giant: clues point to a large hidden population of symbiotic stars
DOI: 10.1093/mnrasl/slw087 Bibcode: 2016MNRAS.461L...1M

Nuñez, N. E.; Nelson, T.; Mukai, K. +6 more

Symbiotic star surveys have traditionally relied almost exclusively on low resolution optical spectroscopy. However, we can obtain a more reliable estimate of their total Galactic population by using all available signatures of the symbiotic phenomenon. Here we report the discovery of a hard X-ray source, 4PBC J0642.9+5528, in the Swift hard X-ray…

2016 Monthly Notices of the Royal Astronomical Society
IUE 54