Search Publications

The mass fraction of AGN and the Fundamental Plane of black hole activity from a large X-ray-selected sample of LINERs
DOI: 10.1093/mnras/stv2450 Bibcode: 2016MNRAS.455.2551N

Best, P. N.; Nisbet, D. M.

A sample of 576 X-ray-selected LINERs was constructed by combining data from the 3XMM-DR4 and SDSS-DR7 catalogues. The sample was used to investigate the fraction of galaxies hosting a LINER, finding that the fraction is a strong function of both stellar mass and black hole mass (increasing as {f_LINER ∝ M^{1.6 ± 0.2}_{*}} and {f_LINER ∝ M^{0.6 ± …

2016 Monthly Notices of the Royal Astronomical Society
XMM-Newton 30
ROSETTA lander Philae: Touch-down reconstruction
DOI: 10.1016/j.pss.2016.02.005 Bibcode: 2016P&SS..125...12R

Roll, Reinhard; Witte, Lars

The landing of the ROSETTA-mission lander Philae on November 12th 2014 on Comet 67 P/Churyumov-Gerasimenko was planned as a descent with passive landing and anchoring by harpoons at touch-down. Actually the lander was not fixed at touch-down to the ground due to failing harpoons. The lander internal damper was actuated at touch-down for 42.6 mm wi…

2016 Planetary and Space Science
Rosetta 30
HST imaging of the dusty filaments and nucleus swirl in NGC4696 at the centre of the Centaurus Cluster
DOI: 10.1093/mnras/stw1350 Bibcode: 2016MNRAS.461..922F

Fabian, A. C.; Reynolds, C. S.; Pinto, C. +14 more

Narrow-band HST imaging has resolved the detailed internal structure of the 10 kpc diameter H α+[N II] emission line nebulosity in NGC4696, the central galaxy in the nearby Centaurus cluster, showing that the dusty, molecular, filaments have a width of about 60 pc. Optical morphology and velocity measurements indicate that the filaments are dragge…

2016 Monthly Notices of the Royal Astronomical Society
XMM-Newton eHST 30
Decimetre-scaled spectrophotometric properties of the nucleus of comet 67P/Churyumov-Gerasimenko from OSIRIS observations
DOI: 10.1093/mnras/stw2511 Bibcode: 2016MNRAS.462S.287F

Jorda, L.; Lamy, P. L.; Bertaux, J. -L. +55 more

We present the results of the photometric and spectrophotometric properties of the 67P/Churyumov-Gerasimenko nucleus derived with the Optical, Spectroscopic and Infrared Remote Imaging System instrument during the closest fly-by over the comet, which took place on 2015 February 14 at a distance of ∼6 km from the surface. Several images covering th…

2016 Monthly Notices of the Royal Astronomical Society
Rosetta 30
Properties of massive star-forming clumps with infall motions
DOI: 10.1093/mnras/stw1301 Bibcode: 2016MNRAS.461.2288H

Zhou, Jian-Jun; Wu, Gang; Esimbek, Jarken +7 more

In this work, we aim to characterize high-mass clumps with infall motions. We selected 327 clumps from the Millimetre Astronomy Legacy Team 90-GHz survey, and identified 100 infall candidates. Combined with the results of He et al., we obtained a sample of 732 high-mass clumps, including 231 massive infall candidates and 501 clumps where infall is…

2016 Monthly Notices of the Royal Astronomical Society
Herschel 30
The Peculiar Debris Disk of HD 111520 as Resolved by the Gemini Planet Imager
DOI: 10.3847/0004-637X/826/2/147 Bibcode: 2016ApJ...826..147D

Matthews, Brenda C.; Duchêne, Gaspard; Oppenheimer, Rebecca +33 more

Using the Gemini Planet Imager, we have resolved the circumstellar debris disk around HD 111520 at a projected range of ∼30-100 AU in both total and polarized H-band intensity. The disk is seen edge-on at a position angle of 165° along the spine of emission. A slight inclination and asymmetric warp are covariant and alter the interpretation of the…

2016 The Astrophysical Journal
Herschel 30
HST-COS Observations of AGNs. III. Spectral Constraints in the Lyman Continuum from Composite COS/G140L Data
DOI: 10.3847/0004-637X/817/1/56 Bibcode: 2016ApJ...817...56T

Stevans, Matthew L.; Shull, J. Michael; Danforth, Charles W. +1 more

The rest-frame ultraviolet (UV) spectra of active galactic nuclei (AGNs) are important diagnostics of both accretion disk physics and their contribution to the metagalactic ionizing UV background. Though the mean AGN spectrum is well characterized with composite spectra at wavelengths greater than 912 Å, the shorter-wavelength extreme-UV (EUV) rem…

2016 The Astrophysical Journal
eHST 30
Mirror mode structures ahead of dipolarization front near the neutral sheet observed by Cluster
DOI: 10.1002/2016GL070382 Bibcode: 2016GeoRL..43.8853W

Zhang, T. L.; Nakamura, R.; Baumjohann, W. +4 more

Magnetic compressional structures ahead of a dipolarization front (DF) on 30 August 2002 are investigated by using Cluster data. Our findings are as follows: (1) the structures, observed near the neutral sheet, are mainly compressional and dominant in BZ; (2) they are almost nonpropagating relative to the local ion bulk flow and their l…

2016 Geophysical Research Letters
Cluster 30
Coronal Hole and Solar Global Magnetic Field Evolution in 1976 - 2012
DOI: 10.1007/s11207-016-0966-2 Bibcode: 2016SoPh..291.2329B

Bilenko, Irina A.; Tavastsherna, Ksenia S.

We study the spatial-temporal evolution of a coronal hole and compare it with that of the solar global magnetic field in Cycles 21 - 23 (1976 - 2012). We also analyze the latitude-longitude distribution dynamics of coronal holes and the regularities in the global magnetic field associated with the solar polar field reversal. Polar and non-polar co…

2016 Solar Physics
SOHO 30
Vetting Galactic Leavitt Law Calibrators Using Radial Velocities: On the Variability, Binarity, and Possible Parallax Error of 19 Long-period Cepheids
DOI: 10.3847/0067-0049/226/2/18 Bibcode: 2016ApJS..226...18A

Holl, B.; Mowlavi, N.; Roelens, M. +9 more

We investigate the radial velocity (RV) variability and spectroscopic binarity of 19 Galactic long-period ({P}{puls} ≳ 10 days) classical Cepheid variable stars whose trigonometric parallaxes are being measured using the Hubble Space Telescope and Gaia. Our primary objective is to constrain possible parallax error due to undetected orbi…

2016 The Astrophysical Journal Supplement Series
eHST 30