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Fitting BICEP2 with defects, primordial gravitational waves and dust
DOI: 10.1088/1742-6596/600/1/012025 Bibcode: 2015JPhCS.600a2025L

Kunz, Martin; Liddle, Andrew R.; Lizarraga, Joanes +3 more

In this work we discuss the possibility of cosmic defects being responsible for the B-mode signal measured by the BICEP2 collaboration. We also allow for the presence of other cosmological sources of B-modes such as inflationary gravitational waves and polarized dust foregrounds, which might contribute to or dominate the signal. On the one hand, w…

2015 Journal of Physics Conference Series
Planck 1
Stochastic acceleration of ions driven by Pc1 wave packets
DOI: 10.1063/1.4926823 Bibcode: 2015PhPl...22g2901K

Sibeck, D. G.; Khazanov, G. V.; Tel'nikhin, A. A. +1 more

The stochastic motion of protons and He+ ions driven by Pc1 wave packets is studied in the context of resonant particle heating. Resonant ion cyclotron heating typically occurs when wave powers exceed 10-4 nT2/Hz. Gyroresonance breaks the first adiabatic invariant and energizes keV ions. Cherenkov resonances with t…

2015 Physics of Plasmas
Cluster 1
Special issue editorial - Plasma interactions with Solar System Objects: Anticipating Rosetta, Maven and Mars Orbiter Mission
DOI: 10.1016/j.pss.2015.11.005 Bibcode: 2015P&SS..119....1C

Coates, A. J.; Yamauchi, M.; Wellbrock, A.

Within our solar system, the planets, moons, comets and asteroids all have plasma interactions. The interaction depends on the nature of the object, particularly the presence of an atmosphere and a magnetic field. Even the size of the object matters through the finite gyroradius effect and the scale height of cold ions of exospheric origin. It als…

2015 Planetary and Space Science
MEx Rosetta VenusExpress 1
The inner ∼ 40 pc radial distribution of the star formation rate for a nearby Seyfert 2 galaxy M51
DOI: 10.1088/1674-4527/15/6/003 Bibcode: 2015RAA....15..802F

Bian, Wei-Hao; He, Zhi-Cheng; Fang, Li-Ling +1 more

We investigate the spatially resolved specific star formation rate (SSFR) in the inner ∼40 pc for a nearby Seyfert 2 galaxy, M51 (NGC 5194) by analyzing spectra obtained with the Hubble Space Telescope (HST) Space Telescope Imaging Spectrograph (STIS). We present 24 radial spectra measured along the STIS long slit in M51, extending ∼ 1″ from the n…

2015 Research in Astronomy and Astrophysics
eHST 1
Ultraviolet spectroscopic investigation of HU Aqr and AN UMa with the data from HST and IUE
DOI: 10.1515/astro-2017-0234 Bibcode: 2015BaltA..24..327S

Sanad, M. R.

We present ultraviolet spectroscopic study of two polar systems, HU Aqr and AN UMa, observed with the Hubble Space Telescope's Space Telescope Imaging Spectrograph (STIS) and Faint Object Spectrograph (FOS) and with the International Ultraviolet Explorer (IUE) during the period 1979--2003, to diagnose the ultraviolet fluxes of C IV 1550 Å and He I…

2015 Baltic Astronomy
IUE eHST 1
Rosetta mission: When the dust has settled
DOI: 10.1038/nphys3245 Bibcode: 2015NatPh..11...96J

Jewitt, David

The Rosetta orbiter following Comet 67P has captured not only the public imagination but also actual dust grains from the comet's nucleus, revealing their composition, morphology and strength.

2015 Nature Physics
Rosetta 1
Introduction to the special issue on Venus exploration
DOI: 10.1016/j.pss.2015.06.003 Bibcode: 2015P&SS..113....1S

Piccioni, G.; Wilson, C.; Svedhem, H.

Venus Express ended its mission in December 2014 after an extraordinary successful eight and a half years at Venus. The first years of the mission concentrated on the original objectives of the mission, namely to study the dynamics, structure and chemistry of the atmosphere, to investigate the plasma environment and its interaction with the solar …

2015 Planetary and Space Science
VenusExpress 1
Constraints on the birth of the universe and origin of cosmic dark flow
DOI: 10.1142/S0217751X15450220 Bibcode: 2015IJMPA..3045022M

Garnavich, P.; Mathews, G. J.; Gangopadhyay, M. R. +4 more

We summarize three recent efforts to constrain the first few moments of cosmic creation before and during the epoch of inflation. We consider two means to explain a slight dip in the power spectrum of the cosmic microwave background for multipoles in the range of ℓ = 10-30 from both the Planck and WMAP data. We show that such a dip could be the re…

2015 International Journal of Modern Physics A
Planck 1
The Science of the Cluster Mission
DOI: 10.1007/978-3-319-18359-6_8 Bibcode: 2015ASSP...41..159T

Laakso, Harri; Goldstein, Melvyn L.; Escoubet, C. Philippe +6 more

2015 Magnetospheric Plasma Physics: The Impact of Jim Dungey's Research
Cluster 1
Consistency relation for natural inflation with Planck 2015 data
DOI: 10.1007/s10509-015-2514-1 Bibcode: 2015Ap&SS.359...63N

Nozari, Kourosh; Kahvaee, H.; Rashidi, N.

We consider the cosine Natural inflation model that is a good candidate to explain the initial accelerating phase of the universe. By computing the inflationary parameters in Einstein frame, we construct a consistency relation between the scalar spectral index, tensor-to-scalar ratio, as well as the running of the scalar spectral index and compare…

2015 Astrophysics and Space Science
Planck 1