Search Publications

The cosmic assembly of stellar haloes in massive early-type Galaxies
DOI: 10.1093/mnras/stw3382 Bibcode: 2017MNRAS.466.4888B

Pérez-González, Pablo G.; Curtis-Lake, Emma; Trujillo, Ignacio +5 more

Using the exquisite depth of the Hubble Ultra Deep Field (HUDF12 programme) data set, we explore the ongoing assembly of the outermost regions of the most massive galaxies (Mstellar ≥ 5× 1010 M) at z ≤ 1. The outskirts of massive objects, particularly early-type Galaxies (ETGs), are expected to suffer a dramatic t…

2017 Monthly Notices of the Royal Astronomical Society
eHST 44
CO-driven Activity in Comet C/2017 K2 (PANSTARRS)
DOI: 10.3847/2041-8213/aa921f Bibcode: 2017ApJ...849L...8M

Chambers, Kenneth C.; Magnier, Eugene; Bauer, James +12 more

Comet C/2017 K2 (PANSTARRS) was discovered by the Pan-STARRS1 (PS1) Survey on 2017 May 21 at a distance of 16.09 au from the Sun, the second most distant discovery of an active comet. Pre-discovery images in the PS1 archive back to 2014 and additional deep CFHT images between 2013 May 10-13 showed the comet to be active at 23.75 au. We derive an u…

2017 The Astrophysical Journal
Rosetta 44
Low mass X-ray binaries in the Inner Galaxy: implications for millisecond pulsars and the GeV excess
DOI: 10.1088/1475-7516/2017/05/056 Bibcode: 2017JCAP...05..056H

Heinke, Craig; Linden, Tim; Haggard, Daryl +1 more

If millisecond pulsars (MSPs) are responsible for the excess gamma-ray emission observed from the region surrounding the Galactic Center, the same region should also contain a large population of low-mass X-ray binaries (LMXBs). In this study, we compile and utilize a sizable catalog of LMXBs observed in the the Milky Way's globular cluster system…

2017 Journal of Cosmology and Astroparticle Physics
INTEGRAL 44
Planck data versus large scale structure: Methods to quantify discordance
DOI: 10.1103/PhysRevD.95.123535 Bibcode: 2017PhRvD..95l3535C

Battye, Richard A.; Moss, Adam; Charnock, Tom

Discordance in the Λ cold dark matter cosmological model can be seen by comparing parameters constrained by cosmic microwave background (CMB) measurements to those inferred by probes of large scale structure. Recent improvements in observations, including final data releases from both Planck and SDSS-III BOSS, as well as improved astrophysical unc…

2017 Physical Review D
Planck 44
Global Mars-solar wind coupling and ion escape
DOI: 10.1002/2017JA024306 Bibcode: 2017JGRA..122.8051R

Barabash, Stas; Nilsson, Hans; Holmström, Mats +2 more

Loss of the early Martian atmosphere is often thought to have occurred due to an effective transfer of the solar wind energy through the Martian induced magnetic barrier to the ionosphere. We have quantified the coupling efficiency by comparing the power of the heavy ion outflow with the available power supplied by the upstream solar wind. Constra…

2017 Journal of Geophysical Research (Space Physics)
MEx 44
The 67P/Churyumov-Gerasimenko observation campaign in support of the Rosetta mission
DOI: 10.1098/rsta.2016.0249 Bibcode: 2017RSPTA.37560249S

Lasue, J.; Villanueva, G. L.; Lara, L. M. +112 more

We present a summary of the campaign of remote observations that supported the European Space Agency's Rosetta mission. Telescopes across the globe (and in space) followed comet 67P/Churyumov-Gerasimenko from before Rosetta's arrival until nearly the end of the mission in September 2016. These provided essential data for mission planning, large-sc…

2017 Philosophical Transactions of the Royal Society of London Series A
Rosetta 44
Binary Central Stars of Planetary Nebulae Discovered Through Photometric Variability. V. The Central Stars of HaTr 7 and ESO 330-9
DOI: 10.3847/1538-3881/153/1/24 Bibcode: 2017AJ....153...24H

Frew, David J.; Reindl, Nicole; Margheim, Steve +3 more

We find the central stars (CSs) of the planetary nebulae (PNe) HaTr 7 and ESO 330-9 to be close-binary systems. Both have orbital periods of less than half a day and contain an irradiated cool companion to the hot CS. We provide light curves, spectra, radial velocity curves, orbital periods, and binary modeling results for both systems. The binary…

2017 The Astronomical Journal
Gaia 44
Discovery of Extended Main-sequence Turnoffs in Four Young Massive Clusters in the Magellanic Clouds
DOI: 10.3847/1538-4357/aa7b36 Bibcode: 2017ApJ...844..119L

Milone, Antonino P.; Deng, Licai; de Grijs, Richard +1 more

An increasing number of young massive clusters (YMCs) in the Magellanic Clouds have been found to exhibit bimodal or extended main sequences (MSs) in their color-magnitude diagrams (CMDs). These features are usually interpreted in terms of a coeval stellar population with different stellar rotational rates, where the blue and red MS stars are popu…

2017 The Astrophysical Journal
eHST 44
Space Weather Effects Produced by the Ring Current Particles
DOI: 10.1007/s11214-017-0412-2 Bibcode: 2017SSRv..212.1315G

Jaynes, Allison; Ganushkina, Natalia; Liemohn, Michael

One of the definitions of space weather describes it as the time-varying space environment that may be hazardous to technological systems in space and/or on the ground and/or endanger human health or life. The ring current has its contributions to space weather effects, both in terms of particles, ions and electrons, which constitute it, and magne…

2017 Space Science Reviews
Cluster 44
Multiplicity and clustering in Taurus star-forming region. I. Unexpected ultra-wide pairs of high-order multiplicity in Taurus
DOI: 10.1051/0004-6361/201629398 Bibcode: 2017A&A...599A..14J

Duchêne, Gaspard; Moraux, Estelle; Joncour, Isabelle


Aims: This work analyses the spatial distribution of stars in Taurus with a specific focus on multiple stars and wide pairs in order to derive new constraints on star formation and early dynamical evolution scenarios.
Methods: We collected the multiplicity data of stars in Taurus to build an up-to-date stellar/multiplicity catalog. We fi…

2017 Astronomy and Astrophysics
Gaia 43