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Micron-sized forsterite grains in the pre-planetary nebula of IRAS 17150-3224. Searching for clues to the mysterious evolution of massive AGB stars
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, …
Strategy to minimize dust foregrounds in B -mode searches
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…
Anomalous Earth flybys of spacecraft
Wilhelm, Klaus; Dwivedi, Bhola N.
A small deviation from the
Far-infrared CO and H2O emission in intermediate-mass protostars
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…
Modelling of the surface emission of the low magnetic field magnetar SGR 0418+5729
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 …
The velocity distribution in the solar neighbourhood from the LAMOST pilot survey
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…
Satellite content and quenching of star formation in galaxy groups at z ~ 1.8
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…
Inflection point inflation and dark energy in supergravity
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…
To what extent can intracrater layered deposits that lack clear sedimentary textures be used to infer depositional environments?
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…
Spectral models for early time SN 2011fe observations
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 …