Search Publications

Micron-sized forsterite grains in the pre-planetary nebula of IRAS 17150-3224. Searching for clues to the mysterious evolution of massive AGB stars
DOI: 10.1051/0004-6361/201424843 Bibcode: 2015A&A...576A..98D

Waters, L. B. F. M.; Blommaert, J. A. D. L.; Min, M. +3 more


Aims: We study the grain properties and location of the forsterite crystals in the circumstellar environment of the pre-planetary nebula (PPN) IRAS 17150-3224 in order to learn more about the as yet poorly understood evolutionary phase prior to the PPN.
Methods: We use the best-fit model for IRAS 17150-3224 of Meixner et al. (2002, ApJ, …

2015 Astronomy and Astrophysics
Herschel ISO 12
Strategy to minimize dust foregrounds in B -mode searches
DOI: 10.1103/PhysRevD.91.081303 Bibcode: 2015PhRvD..91h1303K

Kovetz, Ely D.; Kamionkowski, Marc

The Planck satellite has identified several patches of sky with low polarized dust emission, obvious targets for searches for the cosmic microwave background B -mode signal from inflationary gravitational waves. Still, given the Planck measurement uncertainties, the polarized dust foregrounds in these different candidate patches may differ by an o…

2015 Physical Review D
Planck 12
Anomalous Earth flybys of spacecraft
DOI: 10.1007/s10509-015-2413-5 Bibcode: 2015Ap&SS.358...18W

Wilhelm, Klaus; Dwivedi, Bhola N.

A small deviation from the 1/r potential is expected for the gravitational interaction of extended bodies. It is explained as a consequence of a recently proposed gravitational impact model (Wilhelm et al. in Astrophy…

2015 Astrophysics and Space Science
Rosetta 12
Far-infrared CO and H2O emission in intermediate-mass protostars
DOI: 10.1051/0004-6361/201526021 Bibcode: 2015A&A...578A..20M

Karska, A.; Fuente, A.; Kristensen, L. E. +4 more

Context. Intermediate-mass young stellar objects (YSOs) provide a link to understanding how feedback from shocks and UV radiation scales from low- to high-mass star forming regions.
Aims: Our aim is to analyze excitation of CO and H2O in deeply embedded intermediate-mass YSOs and compare it with similar studies on low-mass and high…

2015 Astronomy and Astrophysics
Herschel 12
Modelling of the surface emission of the low magnetic field magnetar SGR 0418+5729
DOI: 10.1093/mnras/stv1535 Bibcode: 2015MNRAS.452.3357G

Rea, N.; Perna, R.; Guillot, S. +2 more

We perform a detailed modelling of the post-outburst surface emission of the low magnetic field magnetar SGR 0418+5729. The dipolar magnetic field of this source, B=6 {× 10^{12}}{ G} estimated from its spin-down rate, is in the observed range of magnetic fields for normal pulsars. The source is further characterized by a high pulse fraction and a …

2015 Monthly Notices of the Royal Astronomical Society
XMM-Newton 12
The velocity distribution in the solar neighbourhood from the LAMOST pilot survey
DOI: 10.1093/mnras/stu2620 Bibcode: 2015MNRAS.447.2367X

Zhang, Yong; Xu, Yan; Mao, Shude +5 more

We use about 15 000 F/G nearby dwarf stars selected from the LAMOST pilot survey to map the U-V velocity distribution in the solar neighbourhood. An extreme deconvolution algorithm is applied to reconstruct an empirical multi-Gaussian model. In addition to the well-known substructures, e.g. Sirius, Coma Berenices, Hyades-Pleiades overdensities, se…

2015 Monthly Notices of the Royal Astronomical Society
Hipparcos 12
Satellite content and quenching of star formation in galaxy groups at z ~ 1.8
DOI: 10.1051/0004-6361/201526274 Bibcode: 2015A&A...581A..56G

Finoguenov, A.; Daddi, E.; Le Floc'h, E. +13 more

We study the properties of satellites in the environment of massive star-forming galaxies at z ~ 1.8 in the COSMOS field, using a sample of 215 galaxies on the main sequence of star formation with an average mass of ~1011M. At z> 1.5, these galaxies typically trace halos of mass ≳1013M. We use optic…

2015 Astronomy and Astrophysics
XMM-Newton 12
Inflection point inflation and dark energy in supergravity
DOI: 10.1103/PhysRevD.91.123502 Bibcode: 2015PhRvD..91l3502G

Guo, Zong-Kuan; Gao, Tie-Jun

We consider an inflection point inflationary model in supergravity with a single chiral superfield and show that the predicted values of the scalar spectral index and tensor-to-scalar ratio are consistent with the Planck 2015 results. In this model supersymmetry is strongly broken after inflation, which results in a non-supersymmetry de Sitter vac…

2015 Physical Review D
Planck 12
To what extent can intracrater layered deposits that lack clear sedimentary textures be used to infer depositional environments?
DOI: 10.1016/j.icarus.2014.11.004 Bibcode: 2015Icar..248..526C

Kah, Linda C.; Cadieux, Sarah B.

Craters within Arabia Terra, Mars, contain hundreds of meters of layered strata showing systematic alternation between slope- and cliff-forming units, suggesting either rhythmic deposition of distinct lithologies or similar lithologies that experienced differential cementation. On Earth, rhythmically deposited strata can be examined in terms of st…

2015 Icarus
MEx 12
Spectral models for early time SN 2011fe observations
DOI: 10.1093/mnras/stv1951 Bibcode: 2015MNRAS.454.2549B

Gal-Yam, A.; Wang, L.; Sullivan, M. +12 more

We use observed UV through near-IR spectra to examine whether SN 2011fe can be understood in the framework of Branch-normal Type Ia supernovae (SNe Ia) and to examine its individual peculiarities. As a benchmark, we use a delayed-detonation model with a progenitor metallicity of Z/20. We study the sensitivity of features to variations …

2015 Monthly Notices of the Royal Astronomical Society
eHST 12