Search Publications

The effect of accretion on the measurement of neutron star mass and radius in the low-mass X-ray binary 4U 1608-52
DOI: 10.1093/mnras/stu1139 Bibcode: 2014MNRAS.442.3777P

Suleimanov, Valery F.; Poutanen, Juri; Nättilä, Joonas +4 more

Spectral measurements of thermonuclear (type I) X-ray bursts from low-mass X-ray binaries have been used to measure neutron star (NS) masses and radii. A number of systematic issues affect such measurements and have raised concerns as to the robustness of the methods. We present analysis of the X-ray emission from bursts observed from 4U 1608-52 a…

2014 Monthly Notices of the Royal Astronomical Society
Exosat 93
Observational constraints on slow-roll inflation coupled to a Gauss-Bonnet term
DOI: 10.1103/PhysRevD.90.063527 Bibcode: 2014PhRvD..90f3527K

Koh, Seoktae; Lee, Bum-Hoon; Lee, Wonwoo +1 more

We study slow-roll inflation with a Gauss-Bonnet term that is coupled to an inflaton field nonminimally. We investigate the inflationary solutions for a specific type of the nonminimal coupling to the Gauss-Bonnet term and inflaton potential both analytically and numerically. We also calculate the observable quantities such as the power spectra of…

2014 Physical Review D
Planck 93
High-resolution, 3D radiative transfer modeling. I. The grand-design spiral galaxy M 51
DOI: 10.1051/0004-6361/201424747 Bibcode: 2014A&A...571A..69D

Lebouteiller, Vianney; Wilson, Christine D.; De Looze, Ilse +20 more

Context. Dust reprocesses about half of the stellar radiation in galaxies. The thermal re-emission by dust of absorbed energy is considered to be driven merely by young stars so is often applied to tracing the star formation rate in galaxies. Recent studies have argued that the old stellar population might be responsible for a non-negligible fract…

2014 Astronomy and Astrophysics
Herschel 93
The Solar Internetwork. I. Contribution to the Network Magnetic Flux
DOI: 10.1088/0004-637X/797/1/49 Bibcode: 2014ApJ...797...49G

Gošić, M.; Bellot Rubio, L. R.; Katsukawa, Y. +2 more

The magnetic network (NE) observed on the solar surface harbors a sizable fraction of the total quiet Sun flux. However, its origin and maintenance are not well known. Here we investigate the contribution of internetwork (IN) magnetic fields to the NE flux. IN fields permeate the interior of supergranular cells and show large emergence rates. We u…

2014 The Astrophysical Journal
Hinode 93
Saturn ring seismology: Evidence for stable stratification in the deep interior of Saturn
DOI: 10.1016/j.icarus.2014.08.006 Bibcode: 2014Icar..242..283F

Fuller, Jim

Seismology allows for direct observational constraints on the interior structures of stars and planets. Recent observations of Saturn's ring system have revealed the presence of density waves within the rings excited by oscillation modes within Saturn, allowing for precise measurements of a limited set of the planet's mode frequencies. We construc…

2014 Icarus
Cassini 92
Reverberation Mapping of the Seyfert 1 Galaxy NGC 7469
DOI: 10.1088/0004-637X/795/2/149 Bibcode: 2014ApJ...795..149P

Motohara, K.; Skowron, D. M.; Skowron, J. +43 more

A large reverberation-mapping study of the Seyfert 1 galaxy NGC 7469 has yielded emission-line lags for Hβ λ4861 and He II λ4686 and a central black hole mass measurement M BH ≈ 1 × 107 M , consistent with previous measurements. A very low level of variability during the monitoring campaign precluded meeting our o…

2014 The Astrophysical Journal
IUE 92
Simultaneous NuSTAR and XMM-Newton 0.5-80 keV spectroscopy of the narrow-line Seyfert 1 galaxy SWIFT J2127.4+5654
DOI: 10.1093/mnras/stu404 Bibcode: 2014MNRAS.440.2347M

Harrison, F. A.; Cappi, M.; Fabian, A. C. +20 more

We present a broad-band spectral analysis of the joint XMM-Newton and Nuclear Spectroscopic Telescope Array observational campaign of the narrow-line Seyfert 1 SWIFT J2127.4+5654, consisting of 300 ks performed during three XMM-Newton orbits. We detect a relativistic broadened iron Kα line originating from the innermost regions of the accretion di…

2014 Monthly Notices of the Royal Astronomical Society
XMM-Newton 92
Rapidly growing black holes and host galaxies in the distant Universe from the Herschel Radio Galaxy Evolution Project
DOI: 10.1051/0004-6361/201323310 Bibcode: 2014A&A...566A..53D

Stern, D.; Bauer, F. E.; Ibar, E. +14 more

We present results from a comprehensive survey of 70 radio galaxies at redshifts 1 <z< 5.2 using the PACS and SPIRE instruments on board the Herschel Space Observatory. Combined with existing mid-IR photometry from the Spitzer Space Telescope, published 870 µm photometry, and new observations obtained with LABOCA on the APEX telescope,…

2014 Astronomy and Astrophysics
Herschel 92
Discovery of a rich proto-cluster at z = 2.9 and associated diffuse cold gas in the VIMOS Ultra-Deep Survey (VUDS)
DOI: 10.1051/0004-6361/201423811 Bibcode: 2014A&A...570A..16C

Maccagni, D.; Cimatti, A.; Ilbert, O. +42 more

High-density environments are crucial places for studying the link between hierarchical structure formation and stellar mass growth in galaxies. In this work, we characterise a massive proto-cluster at z = 2.895 that we found in the COSMOS field using the spectroscopic sample of the VIMOS Ultra-Deep Survey (VUDS). This is one of the rare structure…

2014 Astronomy and Astrophysics
eHST 92
The extended ROSAT-ESO Flux Limited X-ray Galaxy Cluster Survey (REFLEX II). IV. X-ray luminosity function and first constraints on cosmological parameters
DOI: 10.1051/0004-6361/201323155 Bibcode: 2014A&A...570A..31B

Collins, Chris A.; Böhringer, Hans; Chon, Gayoung

The X-ray luminosity function that is closely related to the cluster mass function is an important statistic of the census of galaxy clusters in our Universe. It is also an important means to probe the cosmological model of our Universe. Based on our recently completed REFLEX II cluster sample comprising 910 galaxy clusters with redshifts we const…

2014 Astronomy and Astrophysics
Planck 92