Search Publications

Long-term Spectral Variability of the Ultraluminous X-Ray Source Holmberg IX X-1
DOI: 10.3847/1538-4357/aa8eeb Bibcode: 2017ApJ...849..121J

Jithesh, V.; Wang, Zhongxiang; Misra, Ranjeev

We investigate the long-term spectral variability in the ultraluminous X-ray source Holmberg IX X-1. By analyzing the data from 8 Suzaku and 13 XMM-Newton observations conducted between 2001 and 2015, we perform a detailed spectral modeling for all spectra with simple models and complex physical models. We find that the spectra can be well explain…

2017 The Astrophysical Journal
Suzaku XMM-Newton 8
Excess entropy and energy feedback from within cluster cores up to r200
DOI: 10.1093/mnras/stx1999 Bibcode: 2017MNRAS.472..713I

Ettori, Stefano; Eckert, Dominique; Majumdar, Subhabrata +3 more

We estimate the 'non-gravitational' entropy-injection profiles, ΔK, and the resultant energy feedback profiles, ΔE, of the intracluster medium for 17 clusters using their Planck Sunyaev-Zel'dovich and ROSAT X-ray observations, spanning a large radial range from 0.2r500 up to r200. The feedback profiles are estimated by compar…

2017 Monthly Notices of the Royal Astronomical Society
Planck 8
Observational study on the fine structure and dynamics of a solar jet. I. Energy build-up process around a satellite spot
DOI: 10.1093/pasj/psx071 Bibcode: 2017PASJ...69...80S

Shibata, Kazunari; Ichimoto, Kiyoshi; Ueno, Satoru +3 more

We report on a solar jet phenomenon associated with successive flares on 2014 November 10. These explosive events were involved with the satellite spots' emergence around a δ-type sunspot in the decaying active region NOAA 12205. The data for this jet were provided by the Solar Dynamics Observatory, the X-Ray Telescope aboard Hinode, and the Inter…

2017 Publications of the Astronomical Society of Japan
Hinode 8
The most massive galaxies in clusters are already fully grown at z ∼ 0.5
DOI: 10.1093/mnras/stw2791 Bibcode: 2017MNRAS.465.2101O

Davies, Roger L.; Houghton, R. C. W.; Oldham, L. J.

By constructing scaling relations for galaxies in the massive cluster MACSJ0717.5 at z = 0.545 and comparing with those of Coma, we model the luminosity evolution of the stellar populations and the structural evolution of the galaxies. We calculate magnitudes, surface brightnesses and effective radii using Hubble Space Telescope (HST)/ACS images a…

2017 Monthly Notices of the Royal Astronomical Society
eHST 8
Occurrence rate of dipolarization fronts in the plasma sheet: Cluster observations
DOI: 10.5194/angeo-35-1015-2017 Bibcode: 2017AnGeo..35.1015X

Plaschke, Ferdinand; Zhang, Tielong; Volwerk, Martin +6 more

We investigate the occurrence rate of dipolarization fronts (DFs) in the plasma sheet by taking full advantage of all four Cluster satellites (C1-4) from years 2001 to 2009. In total, we select 466 joint-observation DF events, in which 318, 282, 254, and 236 DFs are observed by C1, C2, C3, and C4, respectively. Our findings are as follows: (1) the…

2017 Annales Geophysicae
Cluster 8
Distance determination method of dust particles using Rosetta OSIRIS NAC and WAC data
DOI: 10.1016/j.pss.2017.04.018 Bibcode: 2017P&SS..143..256D

Jorda, L.; Lara, L. M.; Bertaux, J. -L. +42 more

The ESA Rosetta spacecraft has been tracking its target, the Jupiter-family comet 67P/Churyumov-Gerasimenko, in close vicinity for over two years. It hosts the OSIRIS instruments: the Optical, Spectroscopic, and Infrared Remote Imaging System composed of two cameras, see e.g. Keller et al. (2007). In some imaging sequences dedicated to observe dus…

2017 Planetary and Space Science
Rosetta 8
Low-frequency oscillatory flow signatures and high-speed flows in the Earth's magnetotail
DOI: 10.1002/2017JA024076 Bibcode: 2017JGRA..122.7042D

Nilsson, H.; Hamrin, M.; Norqvist, P. +6 more

Using plasma sheet data from Cluster 1 spacecraft from 2001 till 2011, we statistically investigate oscillatory signatures in the plasma bulk flow. These periodic oscillations are compared to high-speed and quiet flows. Periodic oscillations are observed approximately 8% of the time, while high-speed flows and quiet flows are observed around 0.5% …

2017 Journal of Geophysical Research (Space Physics)
Cluster 8
INRRI-EDM/2016: the first laser retroreflector on the surface of Mars
DOI: 10.1016/j.asr.2016.10.011 Bibcode: 2017AdSpR..59..645D

Marchetti, E.; Flamini, E.; Mugnuolo, R. +18 more

During Summer 2015 the SCF_Lab (Satellite/lunar/GNSS laser ranging/altimetry and cube/microsat Characterization Facilities Laboratory, http://www.lnf.infn.it/esperimenti/etrusco, Team of INFN-LNF, with support by ASI, carried out an intense activity of final design, manufacturing and testing in order to construct, space qualify and finally integra…

2017 Advances in Space Research
ExoMars-16 8
Relation between the parameters of dust and of molecular and atomic gas in extragalactic star-forming regions
DOI: 10.1134/S1063772917070083 Bibcode: 2017ARep...61..646S

Smirnova, K. I.; Wiebe, D. S.; Sobolev, A. M. +1 more

The relationships between atomic and molecular hydrogen and dust of various sizes in extragalactic star-forming regions are considered, based on observational data from the Spitzer and Herschel infrared space telescopes, the Very Large Array (atomic hydrogen emission) and IRAM (CO emission). The source sample consists of approximately 300 star-for…

2017 Astronomy Reports
Herschel 8
Starburst-driven Superwinds in Quasar Host Galaxies
DOI: 10.3847/2041-8213/aa7631 Bibcode: 2017ApJ...843L..16B

Haas, Martin; Barthel, Peter; Wilkes, Belinda +1 more

During the past five decades astronomers have been puzzled by the presence of strong absorption features including metal lines, observed in the optical and ultraviolet spectra of quasars, signaling inflowing and outflowing gas winds with relative velocities up to several thousands of km s-1. In particular, the location of these winds—cl…

2017 The Astrophysical Journal
Herschel 8