Search Publications

3D Magnetohydrodynamic Models of Nonthermal Photon Emission in the Binary System γ 2 Velorum
DOI: 10.3847/1538-4357/aa876d Bibcode: 2017ApJ...847...40R

Reimer, A.; Reimer, O.; Kissmann, R. +1 more

Recent reports claiming an association of the massive star binary system {γ }2 Velorum (WR 11) with a high-energy γ-ray source observed by Fermi-LAT contrast the so far exclusive role of η Carinae as the hitherto only detected γ-ray emitter in the source class of particle-accelerating colliding-wind binary (CWB) systems. We offer suppor…

2017 The Astrophysical Journal
INTEGRAL 16
Discovery of a 26.2 day period in the long-term X-ray light curve of SXP 1323: a very short orbital period for a long spin period pulsar
DOI: 10.1051/0004-6361/201629299 Bibcode: 2017A&A...602A..81C

Haberl, F.; Sturm, R.; Carpano, S.

Context. About 120 Be/X-ray binaries (BeXBs) are known in the Small Magellanic Cloud (SMC); about half of them are pulsating with periods from a few to hundreds of seconds. SXP 1323 is one of the longest-period pulsars known in this galaxy.
Aims: SXP 1323 is in the field of view of a large set of calibration observations that we analyse syste…

2017 Astronomy and Astrophysics
Suzaku XMM-Newton 16
Constraining the thin disc initial mass function using Galactic classical Cepheids
DOI: 10.1051/0004-6361/201629464 Bibcode: 2017A&A...599A..17M

Lemasle, B.; Figueras, F.; Mor, R. +1 more

Context. The initial mass function (IMF) plays a crucial role in galaxy evolution and its implications on star formation theory make it a milestone for the next decade. It is in the intermediate and high mass ranges where the uncertainties of the IMF are larger. This is a major subject of debate and analysis both for Galactic and extragalactic sci…

2017 Astronomy and Astrophysics
Hipparcos 16
Behind the dust curtain: the spectacular case of GRB 160623A
DOI: 10.1093/mnras/stx2062 Bibcode: 2017MNRAS.472.1465P

Salvaterra, R.; Tiengo, A.; Mereghetti, S. +6 more

We report on the X-ray dust-scattering features observed around the afterglow of the gamma-ray burst GRB 160623A. With an XMM-Newton observation carried out ∼2 d after the burst, we found evidence of at least six rings, with angular size expanding between ∼2 and 9 arcmin, as expected for X-ray scattering of the prompt gamma-ray burst (GRB) emissio…

2017 Monthly Notices of the Royal Astronomical Society
XMM-Newton 16
EXTraS discovery of two pulsators in the direction of the LMC: a Be/X-ray binary pulsar in the LMC and a candidate double-degenerate polar in the foreground
DOI: 10.1051/0004-6361/201629744 Bibcode: 2017A&A...598A..69H

Salvaterra, R.; Haberl, F.; Tiengo, A. +10 more

Context. The Exploring the X-ray Transient and variable Sky (EXTraS) project searches for coherent signals in the X-ray archival data of XMM-Newton.
Aims: XMM-Newton performed more than 400 pointed observations in the region of the Large Magellanic Cloud (LMC). We inspected the results of the EXTraS period search to systematically look for ne…

2017 Astronomy and Astrophysics
XMM-Newton 16
Fan Loops Observed by IRIS, EIS, and AIA
DOI: 10.3847/1538-4357/835/2/244 Bibcode: 2017ApJ...835..244G

Solanki, Sami K.; Polito, Vanessa; Gupta, G. R. +3 more

A comprehensive study of the physical parameters of active region fan loops is presented using the observations recorded with the Interface Region Imaging Spectrometer (IRIS), the EUV Imaging Spectrometer (EIS) on board Hinode, and the Atmospheric Imaging Assembly (AIA) and the Helioseismic and Magnetic Imager (HMI) on board the Solar Dynamics Obs…

2017 The Astrophysical Journal
Hinode IRIS 16
Globular clusters in the far-ultraviolet: evidence for He-enriched second populations in extragalactic globular clusters?
DOI: 10.1093/mnras/stw2382 Bibcode: 2017MNRAS.464..713P

Kundu, Arunav; Zepf, Stephen E.; Peacock, Mark B. +1 more

We investigate the integrated far-ultraviolet (FUV) emission from globular clusters. We present new FUV photometry of M87's clusters based on archival Hubble Space Telescope (HST) Wide Field Planetary Camera 2 F170W observations. We use these data to test the reliability of published photometry based on HST space telescope imaging spectrograph FUV…

2017 Monthly Notices of the Royal Astronomical Society
eHST 16
OH Survey along Sightlines of Galactic Observations of Terahertz C+
DOI: 10.3847/1538-4357/aa67e9 Bibcode: 2017ApJ...839....8T

Wang, Shen; Heiles, Carl; Li, Di +9 more

We have obtained OH spectra of four transitions in the {}2{{{\Pi }}}3/2 ground state, at 1612, 1665, 1667, and 1720 MHz, toward 51 sightlines that were observed in the Herschel project Galactic Observations of Terahertz C+. The observations cover the longitude range of (32°, 64°) and (189°, 207°) in the northern Galactic plan…

2017 The Astrophysical Journal
Herschel 16
X-ray-emitting active galactic nuclei from z = 0.6 to 1.3 in the intermediate- and high-density environments of the ORELSE survey
DOI: 10.1093/mnras/stw3091 Bibcode: 2017MNRAS.466..496R

Tomczak, A.; Fassnacht, C. D.; Kocevski, D. D. +8 more

We studied active galactic nucleus (AGN) activity in 12 large-scale structures (LSSs) in the Observations of Redshift Evolution in Large-Scale Environments (ORELSE) survey, at 0.65 < z < 1.28, using a combination of Chandra observations, optical and NIR imaging and spectroscopy. We located a total of 61 AGNs that were successfully matched to…

2017 Monthly Notices of the Royal Astronomical Society
eHST 16
Results from a triple chord stellar occultation and far-infrared photometry of the trans-Neptunian object (229762) 2007 UK126
DOI: 10.1051/0004-6361/201628620 Bibcode: 2017A&A...600A..12S

Kiss, C.; Ortiz, J. L.; Braga-Ribas, F. +8 more

Context. A stellar occultation by a trans-Neptunian object (TNO) provides an opportunity to probe the size and shape of these distant solar system bodies. In the past seven years, several occultations by TNOs have been observed, but mostly from a single location. Only very few TNOs have been sampled simultaneously from multiple locations. Sufficie…

2017 Astronomy and Astrophysics
Gaia Herschel eHST 16