Search Publications

A Massive Shell of Supernova-formed Dust in SNR G54.1+0.3
DOI: 10.3847/1538-4357/836/1/129 Bibcode: 2017ApJ...836..129T

Gelfand, Joseph D.; Temim, Tea; Reynolds, Stephen P. +5 more

While theoretical models of dust condensation predict that most refractory elements produced in core-collapse supernovae (SNe) efficiently condense into dust, a large quantity of dust has so far only been observed in SN 1987A. We present an analysis of observations from the Spitzer Space Telescope, Herschel Space Observatory, Stratospheric Observa…

2017 The Astrophysical Journal
AKARI Herschel 65
Dust-trapping Vortices and a Potentially Planet-triggered Spiral Wake in the Pre-transitional Disk of V1247 Orionis
DOI: 10.3847/2041-8213/aa8edc Bibcode: 2017ApJ...848L..11K

Monnier, John D.; Kraus, Stefan; Wisniewski, John +9 more

The radial drift problem constitutes one of the most fundamental problems in planet formation theory, as it predicts particles to drift into the star before they are able to grow to planetesimal size. Dust-trapping vortices have been proposed as a possible solution to this problem, as they might be able to trap particles over millions of years, al…

2017 The Astrophysical Journal
Gaia 64
X-Rays from the Location of the Double-humped Transient ASASSN-15lh
DOI: 10.3847/1538-4357/836/1/25 Bibcode: 2017ApJ...836...25M

Sbarufatti, B.; Berger, E.; Dall'Osso, S. +13 more

We present the detection of persistent soft X-ray radiation with {L}x∼ {10}41-1042 erg s-1 at the location of the extremely luminous, double-humped transient ASASSN-15lh as revealed by Chandra and Swift. We interpret this finding in the context of observations from our multiwavelength campaign, which rev…

2017 The Astrophysical Journal
XMM-Newton 64
Dual Maxwellian-Kappa modeling of the solar wind electrons: new clues on the temperature of Kappa populations
DOI: 10.1051/0004-6361/201630194 Bibcode: 2017A&A...602A..44L

Fichtner, H.; Pierrard, V.; Lazar, M. +2 more

Context. Recent studies on Kappa distribution functions invoked in space plasma applications have emphasized two alternative approaches that may assume the temperature parameter either dependent or independent of the power-index κ. Each of them can obtain justification in different scenarios involving Kappa-distributed plasmas, but direct evidence…

2017 Astronomy and Astrophysics
Cluster 64
CMB Polarization B-mode Delensing with SPTpol and Herschel
DOI: 10.3847/1538-4357/aa82bb Bibcode: 2017ApJ...846...45M

Bock, J. J.; Chiang, H. C.; Conley, A. +60 more

We present a demonstration of delensing the observed cosmic microwave background (CMB) B-mode polarization anisotropy. This process of reducing the gravitational-lensing-generated B-mode component will become increasingly important for improving searches for the B modes produced by primordial gravitational waves. In this work, we delens B-mode map…

2017 The Astrophysical Journal
Herschel Planck 64
Nonequilibrium Processes in the Solar Corona, Transition Region, Flares, and Solar Wind (Invited Review)
DOI: 10.1007/s11207-017-1125-0 Bibcode: 2017SoPh..292..100D

Krucker, Säm; Meyer-Vernet, Nicole; Del Zanna, Giulio +12 more

We review the presence and signatures of the non-equilibrium processes, both non-Maxwellian distributions and non-equilibrium ionization, in the solar transition region, corona, solar wind, and flares. Basic properties of the non-Maxwellian distributions are described together with their influence on the heat flux as well as on the rates of indivi…

2017 Solar Physics
IRIS Ulysses 64
iPTF 16asu: A Luminous, Rapidly Evolving, and High-velocity Supernova
DOI: 10.3847/1538-4357/aa99de Bibcode: 2017ApJ...851..107W

Cenko, S. B.; Sollerman, J.; Hurley, K. +23 more

Wide-field surveys are discovering a growing number of rare transients whose physical origin is not yet well understood. Here we present optical and UV data and analysis of intermediate Palomar Transient Factory (iPTF) 16asu, a luminous, rapidly evolving, high-velocity, stripped-envelope supernova (SN). With a rest-frame rise time of just four day…

2017 The Astrophysical Journal
INTEGRAL 64
Molecular gas on large circumgalactic scales at z = 3.47
DOI: 10.1093/mnras/stx712 Bibcode: 2017MNRAS.468.3468G

Maiolino, R.; Marconi, A.; Ginolfi, M. +9 more

We report the ALMA observations of the most massive (star-forming) galaxy in the redshift range 3 < z < 4 within the whole Great Observatories Origins Deep Survey South field (GOODS-S) field. We detect a large elongated structure of molecular gas around the massive primeval galaxy, traced by the CO(4-3) emission, and extended over 40 kpc. We…

2017 Monthly Notices of the Royal Astronomical Society
eHST 64
Cross-correlating Planck tSZ with RCSLenS weak lensing: implications for cosmology and AGN feedback
DOI: 10.1093/mnras/stx1659 Bibcode: 2017MNRAS.471.1565H

Heymans, Catherine; Hinshaw, Gary; Harnois-Déraps, Joachim +11 more

We present measurements of the spatial mapping between (hot) baryons and the total matter in the Universe, via the cross-correlation between the thermal Sunyaev-Zeldovich (tSZ) map from Planck and the weak gravitational lensing maps from the Red Cluster Sequence Lensing Survey (RCSLenS). The cross-correlations are performed on the map level where …

2017 Monthly Notices of the Royal Astronomical Society
Planck 64
The Gaia-ESO Survey: Calibration strategy
DOI: 10.1051/0004-6361/201629450 Bibcode: 2017A&A...598A...5P

Gilmore, G.; Bayo, A.; Allende Prieto, C. +60 more

The Gaia-ESO survey (GES) is now in its fifth and last year of observations and has produced tens of thousands of high-quality spectra of stars in all Milky Way components. This paper presents the strategy behind the selection of astrophysical calibration targets, ensuring that all GES results on radial velocities, atmospheric parameters, and chem…

2017 Astronomy and Astrophysics
Gaia 64