Search Publications

Disentangling the ISM phases of the dwarf galaxy NGC 4214 using [C II] SOFIA/GREAT observations
DOI: 10.1051/0004-6361/201629341 Bibcode: 2017A&A...599A...9F

Lebouteiller, V.; Madden, S. C.; Abel, N. P. +9 more

Context. The [C II] 158 µm fine structure line is one of the dominant cooling lines in the interstellar medium (ISM) and is an important tracer of star formation. Recent velocity-resolved studies with Herschel/HIFI and SOFIA/GREAT showed that the [C II] line can constrain the properties of the ISM phases in star-forming regions. The [C II] l…

2017 Astronomy and Astrophysics
Herschel 21
CMB and matter power spectra with non-linear dark-sector interactions
DOI: 10.1088/1475-7516/2017/01/050 Bibcode: 2017JCAP...01..050V

vom Marttens, R. F.; Casarini, L.; Hipólito-Ricaldi, W. S. +1 more

An interaction between dark matter and dark energy, proportional to the product of their energy densities, results in a scaling behavior of the ratio of these densities with respect to the scale factor of the Robertson-Walker metric. This gives rise to a class of cosmological models which deviate from the standard model in an analytically tractabl…

2017 Journal of Cosmology and Astroparticle Physics
Planck 21
Investigating the physical properties of outbursts on comet 67P/Churyumov-Gerasimenko
DOI: 10.1093/mnras/stx2768 Bibcode: 2017MNRAS.469S.731L

Jorda, L.; Lamy, P. L.; Lara, L. M. +46 more

Cometary outbursts on several comets have been observed both by ground-based telescopes and by in situ instruments on spacecraft. However, the mechanism behind these phenomena and their physical properties are still unclear. The optical, spectrocopic and infrared remote imaging system (OSIRIS) onboard the Rosetta spacecraft provided first-hand inf…

2017 Monthly Notices of the Royal Astronomical Society
Rosetta 21
Active Longitude and Coronal Mass Ejection Occurrences
DOI: 10.3847/1538-4357/aa62a8 Bibcode: 2017ApJ...838...18G

Srivastava, A. K.; Erdélyi, R.; Singh, T. +2 more

The spatial inhomogeneity of the distribution of coronal mass ejection (CME) occurrences in the solar atmosphere could provide a tool to estimate the longitudinal position of the most probable CME-capable active regions in the Sun. The anomaly in the longitudinal distribution of active regions themselves is often referred to as active longitude (A…

2017 The Astrophysical Journal
SOHO 21
A new solar wind-driven global dynamic plasmapause model: 1. Database and statistics
DOI: 10.1002/2017JA023912 Bibcode: 2017JGRA..122.7153Z

Liemohn, Michael W.; Gallagher, Dennis L.; He, Fei +5 more

A large database, possibly the largest plasmapause location database, with 49,119 plasmapause crossing events from the in situ observations and 3957 plasmapause profiles (corresponding to 48,899 plasmapause locations in 1 h magnetic local time (MLT) intervals) from optical remote sensing from 1977 to 2015 by 18 satellites is compiled. The response…

2017 Journal of Geophysical Research (Space Physics)
Cluster 21
Hubble Space Telescope astrometry of the closest brown dwarf binary system - I. Overview and improved orbit
DOI: 10.1093/mnras/stx1177 Bibcode: 2017MNRAS.470.1140B

Apai, D.; Pourbaix, D.; Bedin, L. R. +4 more

Located at 2 pc, the L7.5+T0.5 dwarfs system WISE J104915.57-531906.1 (Luhman 16 AB) is the third closest system known to Earth, making it a key benchmark for detailed investigation of brown dwarf atmospheric properties, thermal evolution, multiplicity, and planet-hosting frequency. In the first study of this series - based on a multicycle Hubble …

2017 Monthly Notices of the Royal Astronomical Society
Gaia eHST 21
Analysis of Local Slopes at the InSight Landing Site on Mars
DOI: 10.1007/s11214-016-0292-x Bibcode: 2017SSRv..211..109F

Kirk, R. L.; Golombek, M. P.; Fergason, R. L. +6 more

To evaluate the topography of the surface within the InSight candidate landing ellipses, we generated Digital Terrain Models (DTMs) at lander scales and those appropriate for entry, descent, and landing simulations, along with orthoimages of both images in each stereopair, and adirectional slope images. These products were used to assess the distr…

2017 Space Science Reviews
MEx 21
Discovery of carbon-rich Miras in the Galactic bulge
DOI: 10.1093/mnras/stx1213 Bibcode: 2017MNRAS.469.4949M

Matsunaga, Noriyuki; Whitelock, Patricia A.; Aydi, Elias +4 more

Only one carbon-rich (C-rich, hereinafter) Mira variable has so far been suggested as a member of the Galactic bulge and this is in a symbiotic system. Here we describe a method for selecting C-rich candidates from an infrared colour-colour diagram, (J - Ks) versus ([9] - [18]). Follow-up low-resolution spectroscopy resulted in the dete…

2017 Monthly Notices of the Royal Astronomical Society
AKARI 21
The AT-LESS CO(1-0) survey of submillimetre galaxies in the Extended Chandra Deep Field South: First results on cold molecular gas in galaxies at z ∼ 2
DOI: 10.1093/mnras/stx156 Bibcode: 2017MNRAS.467.1222H

Thomson, A. P.; Ivison, R. J.; Smail, Ian +13 more

We present the first results from our ongoing Australia Telescope Compact Array survey of 12CO(1-0) in Atacama Large Millimeter Array (ALMA)-identified submillimetre galaxies (SMGs) in the Extended Chandra Deep Field South. Strong detections of 12CO(1-0) emission from two SMGs, ALESS 122.1 (z = 2.0232) and ALESS 67.1 (z = 2.1…

2017 Monthly Notices of the Royal Astronomical Society
eHST 21
The Close AGN Reference Survey (CARS). Mrk 1018 halts dimming and experiences strong short-term variability
DOI: 10.1051/0004-6361/201731967 Bibcode: 2017A&A...607L...9K

Combes, F.; Scharwächter, J.; Eckart, A. +12 more

After changing optical AGN type from 1.9 to 1 in 1984, the AGN Mrk 1018 recently reverted back to its type 1.9 state. Our ongoing monitoring now reveals that the AGN has halted its dramatic dimming, reaching a minimum around October 2016. The minimum was followed by an outburst rising with 0.25 U-band mag/month. The rebrightening lasted at least u…

2017 Astronomy and Astrophysics
eHST 21