Search Publications

Far-infrared/submillimetre properties of pre-stellar cores L1521E, L1521F and L1689B as revealed by the Herschel SPIRE instrument - I. Central positions
DOI: 10.1093/mnras/stw428 Bibcode: 2016MNRAS.458.2150M

Abergel, A.; Ward-Thompson, D.; van der Wiel, M. H. D. +5 more

Dust grains play a key role in the physics of star-forming regions, even though they constitute only ∼1 per cent of the mass of the interstellar medium. The derivation of accurate dust parameters such as temperature (Td), emissivity spectral index (β) and column density requires broad-band continuum observations at far-infrared waveleng…

2016 Monthly Notices of the Royal Astronomical Society
Herschel 11
On the Relation between the Mysterious 21 µm Emission Feature of Post-asymptotic Giant Branch Stars and Their Mass-loss Rates
DOI: 10.3847/0004-637X/825/1/68 Bibcode: 2016ApJ...825...68M

Li, Aigen; Jiang, B. W.; Mishra, Ajay

Over two decades ago, a prominent, mysterious emission band peaking at ∼20.1 µm was serendipitously detected in four preplanetary nebulae (PPNe; also known as “protoplanetary nebulae”). To date, this spectral feature, designated as the “21 µm” feature, has been seen in 27 carbon-rich PPNe in the Milky Way and the Magellanic Clouds. The…

2016 The Astrophysical Journal
AKARI ISO 11
Herschel-HIFI view of mid-IR quiet massive protostellar objects
DOI: 10.1051/0004-6361/201527786 Bibcode: 2016A&A...587A.139H

Braine, J.; Bontemps, S.; van Dishoeck, E. F. +9 more


Aims: We present Herschel/HIFI observations of 14 water lines in a small sample of Galactic massive protostellar objects: NGC 6334I(N), DR21(OH), IRAS 16272-4837, and IRAS 05358+3543. Using water as a tracer of the structure and kinematics, we individually study each of these objects with the aim to estimate the amount of water around them, b…

2016 Astronomy and Astrophysics
Herschel 11
Modelling the structure of molecular clouds - I. A multiscale energy equipartition
DOI: 10.1093/mnras/stw781 Bibcode: 2016MNRAS.459.2432V

Klessen, Ralf S.; Veltchev, Todor V.; Donkov, Sava

We present a model for describing the general structure of molecular clouds (MCs) at early evolutionary stages in terms of their mass-size relationship. Sizes are defined through threshold levels at which equipartitions between gravitational, turbulent and thermal energy |W| ∼ f(Ekin + Eth) take place, adopting interdependent…

2016 Monthly Notices of the Royal Astronomical Society
Planck 11
A new model of the microwave polarized sky for CMB experiments
DOI: 10.1093/mnras/stw1787 Bibcode: 2016MNRAS.462.2063H

Bonaldi, Anna; Brown, Michael L.; Hervías-Caimapo, Carlos

We present a new model of the microwave sky in polarization that can be used to simulate data from cosmic microwave background polarization experiments. We exploit the most recent results from the Planck satellite to provide an accurate description of the diffuse polarized foreground synchrotron and thermal dust emission. Our model can include the…

2016 Monthly Notices of the Royal Astronomical Society
Planck 11
The SESAME/CASSE instrument listening to the MUPUS PEN insertion phase on comet 67P/Churyumov-Gerasimenko
DOI: 10.1016/j.actaastro.2016.02.018 Bibcode: 2016AcAau.125..234K

Schmidt, W.; Knollenberg, J.; Knapmeyer, M. +7 more

After the final landing of Philae at the Abydos site on comet 67/P Churyumov-Gerasimenko, the MUPUS (Multipurpose Sensors for Surface and Sub-Surface Science) device started hammering itself into the cometary ground on 14th November 2014, and continued hammering for more than 3 h. During this period, the CASSE (Comet Acoustic Surface Sounding Expe…

2016 Acta Astronautica
Rosetta 11
A large active wave trapped in Jupiter's equator
DOI: 10.1051/0004-6361/201526197 Bibcode: 2016A&A...586A.154L

Sánchez-Lavega, A.; García-Melendo, E.; Gómez-Forrellad, J. M. +2 more

Context. A peculiar atmospheric feature was observed in the equatorial zone (EZ) of Jupiter between September and December 2012 in ground-based and Hubble Space Telescope (HST) images. This feature consisted of two low albedo Y-shaped cloud structures (Y1 and Y2) oriented along the equator and centred on it (latitude 0.5°-1°N).
Aims: We wante…

2016 Astronomy and Astrophysics
eHST 11
Near-infrared Circular and Linear Polarimetry of Monoceros R2
DOI: 10.3847/0004-6256/152/3/67 Bibcode: 2016AJ....152...67K

Kwon, Jungmi; Nagata, Tetsuya; Tamura, Motohide +2 more

We have conducted simultaneous JHK s -band imaging circular and linear polarimetry of the Monoceros R2 (Mon R2) cluster. We present results from deep and wide near-infrared linear polarimetry of the Mon R2 region. Prominent and extended polarized nebulosities over the Mon R2 field are revisited, and an infrared reflection nebula associ…

2016 The Astronomical Journal
eHST 11
Additional spectroscopic redshift measurements for galaxy clusters from the first Planck catalogue
DOI: 10.1134/S1063773716020055 Bibcode: 2016AstL...42...63V

Aghanim, N.; Melnikov, S. S.; Irtuganov, E. N. +10 more

We present the results of spectroscopic redshift measurements for the galaxy clusters from the first all-sky Planck catalogue that have been mostly identified based on the optical observations performed previously by our team (Planck Collaboration 2015a). Data on 13 galaxy clusters at redshifts from z ≈ 0.2 to z ≈ 0.8, including the improved ident…

2016 Astronomy Letters
Planck 11
Minute pulsations in microwaves and X-rays during the flare on May 6, 2005
DOI: 10.1016/j.asr.2016.01.012 Bibcode: 2016AdSpR..57.1456K

Kupriyanova, E. G.; Ratcliffe, H.

Quasi-periodic pulsations are a common feature in the emission associated with solar flares. In particular, pulsations with periods of tens of seconds to a few minutes are often seen in microwave and hard X-ray emission. We examine the spatial and temporal structure of the emission during the flare on May 6, 2005. The source of the flare is a magn…

2016 Advances in Space Research
SOHO 11