Search Publications

Massive stars on the verge of exploding: the properties of oxygen sequence Wolf-Rayet stars
DOI: 10.1051/0004-6361/201425390 Bibcode: 2015A&A...581A.110T

Kaper, L.; de Mink, S. E.; de Koter, A. +7 more

Context. Oxygen sequence Wolf-Rayet (WO) stars are a very rare stage in the evolution of massive stars. Their spectra show strong emission lines of helium-burning products, in particular highly ionized carbon and oxygen. The properties of WO stars can be used to provide unique constraints on the (post-)helium burning evolution of massive stars, an…

2015 Astronomy and Astrophysics
eHST 61
Multi-wavelength observations of the binary system PSR B1259-63/LS 2883 around the 2014 periastron passage
DOI: 10.1093/mnras/stv1988 Bibcode: 2015MNRAS.454.1358C

Krivonos, R.; Tsygankov, S.; Tomsick, J. A. +16 more

We report on the results of the extensive multi-wavelength campaign from optical to GeV γ-rays of the 2014 periastron passage of PSR B1259-63, which is a unique high-mass γ-ray emitting binary system with a young pulsar companion. Observations demonstrate the stable nature of the post-periastron GeV flare and prove the coincidence of the flare wit…

2015 Monthly Notices of the Royal Astronomical Society
INTEGRAL XMM-Newton 61
The Destruction of the Circumstellar Ring of SN 1987A
DOI: 10.1088/2041-8205/806/1/L19 Bibcode: 2015ApJ...806L..19F

Smith, Nathan; Garnavich, Peter; Pun, Chun S. J. +23 more

We present imaging and spectroscopic observations with Hubble Space Telescope and Very Large Telescope of the ring of SN 1987A from 1994 to 2014. After an almost exponential increase of the shocked emission from the hotspots up to day ∼8000 (∼2009), both this and the unshocked emission are now fading. From the radial positions of the hotspots we s…

2015 The Astrophysical Journal
eHST 61
On the origin of magnetosheath plasmoids and their relation to magnetosheath jets
DOI: 10.1002/2015JA021487 Bibcode: 2015JGRA..120.7390K

Gunell, H.; Nilsson, H.; Hamrin, M. +4 more

We investigate localized magnetosheath and solar wind density enhancements, associated with clear magnetic field changes, and therefore referred to as magnetosheath/solar wind plasmoids, respectively. Using Cluster data, we show that there are two distinct populations of magnetosheath plasmoids, one associated with a decrease of magnetic field str…

2015 Journal of Geophysical Research (Space Physics)
Cluster 61
Suzaku X-ray study of the double radio relic galaxy cluster CIZA J2242.8+5301
DOI: 10.1051/0004-6361/201425209 Bibcode: 2015A&A...582A..87A

Kaastra, J. S.; van Weeren, R. J.; Brüggen, M. +7 more

Context. We present the results from Suzaku observations of the merging cluster of galaxies CIZA J2242.8+5301 at z = 0.192.
Aims: To study the physics of gas heating and particle acceleration in cluster mergers, we investigated the X-ray emission from CIZA J2242.8+5301, which hosts two giant radio relics …

2015 Astronomy and Astrophysics
Suzaku XMM-Newton 61
Detecting dark matter substructures around the Milky Way with Gaia
DOI: 10.1093/mnras/stu2147 Bibcode: 2015MNRAS.446.1000F

Feldmann, Robert; Spolyar, Douglas

Cold dark matter (CDM) theory, a pillar of modern cosmology and astrophysics, predicts the existence of a large number of starless dark matter haloes surrounding the Milky Way (MW). However, clear observational evidence of these `dark' substructures remains elusive. Here, we present a detection method based on the small, but detectable, velocity c…

2015 Monthly Notices of the Royal Astronomical Society
Gaia 61
Herschel-ATLAS: the surprising diversity of dust-selected galaxies in the local submillimetre Universe
DOI: 10.1093/mnras/stv1276 Bibcode: 2015MNRAS.452..397C

Ivison, R. J.; de Zotti, G.; Baes, M. +20 more

We present the properties of the first 250 µm blind sample of nearby galaxies (15 < D < 46 Mpc) containing 42 objects from the Herschel Astrophysical Terahertz Large Area Survey. Herschel's sensitivity probes the faint end of the dust luminosity function for the first time, spanning a range of stellar mass (7.4 < M < …

2015 Monthly Notices of the Royal Astronomical Society
Herschel 61
The identification of dust heating mechanisms in nearby galaxies using Herschel 160/250 and 250/350 µm surface brightness ratios
DOI: 10.1093/mnras/stu1841 Bibcode: 2015MNRAS.448..135B

Boquien, M.; Bianchi, S.; Fritz, J. +15 more

We examined variations in the 160/250 and 250/350 µm surface brightness ratios within 24 nearby (<30 Mpc) face-on spiral galaxies observed with the Herschel Space Observatory to identify the heating mechanisms for dust emitting at these wavelengths. The analysis consisted of both qualitative and quantitative comparisons of the 160/250 and…

2015 Monthly Notices of the Royal Astronomical Society
Herschel 61
Does the Presence of Planets Affect the Frequency and Properties of Extrasolar Kuiper Belts? Results from the Herschel Debris and Dunes Surveys
DOI: 10.1088/0004-637X/801/2/143 Bibcode: 2015ApJ...801..143M

Duchêne, G.; Eiroa, C.; Marshall, J. P. +14 more

The study of the planet-debris disk connection can shed light on the formation and evolution of planetary systems and may help “predict” the presence of planets around stars with certain disk characteristics. In preliminary analyses of subsamples of the Herschel DEBRIS and DUNES surveys, Wyatt et al. and Marshall et al. identified a tentative corr…

2015 The Astrophysical Journal
Herschel 61
The Comptonization of accretion disc X-ray emission: consequences for X-ray reflection and the geometry of AGN coronae
DOI: 10.1093/mnras/stu2524 Bibcode: 2015MNRAS.448..703W

Gallo, L. C.; Wilkins, D. R.

We consider the Comptonization of the photons that make up the relativistically blurred reflection that is commonly detected from the accretion discs of active galactic nuclei by the coronae of energetic particles believed to give rise to the powerful X-ray continua by the inverse-Compton scattering of thermal seed photons from the disc. Recent me…

2015 Monthly Notices of the Royal Astronomical Society
XMM-Newton 61