Search Publications

Hubble Space Telescope Ultraviolet Light Curves Reveal Interesting Properties of CC Sculptoris and RZ Leonis
DOI: 10.3847/1538-3881/aa5c88 Bibcode: 2017AJ....153..123S

Szkody, Paula; Sion, Edward M.; Godon, Patrick +6 more

Time-tag ultraviolet data obtained on the Hubble Space Telescope in 2013 reveal interesting variability related to the white dwarf spin in the two cataclysmic variables RZ Leo and CC Scl. RZ Leo shows a period at 220 s and its harmonic at 110 s, thus identifying it as a likely Intermediate Polar (IP). The spin signal is not visible in a short sing…

2017 The Astronomical Journal
eHST 8
Panchromatic spectral energy distributions of simulated galaxies: results at redshift z = 0
DOI: 10.1093/mnras/stx869 Bibcode: 2017MNRAS.469.3775G

Annunziatella, Marianna; Obreja, Aura; Granato, Gian Luigi +5 more

We present predictions of spectral energy distributions (SEDs), from the UV to the FIR, of simulated galaxies at z = 0. These were obtained by post-processing the results of an N-body+hydro simulation of a cosmological box of side 25 Mpc, which uses the Multi-Phase Particle Integrator (MUPPI) for star formation and stellar feedback, with the grasi…

2017 Monthly Notices of the Royal Astronomical Society
Herschel 8
Propagation Characteristics of Two Coronal Mass Ejections from the Sun Far into Interplanetary Space
DOI: 10.3847/1538-4357/aa5ea3 Bibcode: 2017ApJ...837....4Z

Wang, Rui; Liu, Ying D.; Hu, Huidong +1 more

Propagation of coronal mass ejections (CMEs) from the Sun far into interplanetary space is not well understood, due to limited observations. In this study we examine the propagation characteristics of two geo-effective CMEs, which occurred on 2005 May 6 and 13, respectively. Significant heliospheric consequences associated with the two CMEs are ob…

2017 The Astrophysical Journal
SOHO Ulysses 8
Study of the progenitor of the magnetar 1E 2259+586 through Suzaku observations of the associated supernova remnant CTB 109
DOI: 10.1093/pasj/psx012 Bibcode: 2017PASJ...69...40N

Enoto, Teruaki; Makishima, Kazuo; Nakano, Toshio +4 more

We present a study of the progenitor of the magnetar 1E 2259+586, from Suzaku observations of the associated supernova remnant CTB 109. The Suzaku spectra, either spatially integrated or spatially resolved, were successfully described by a two-component plasma model, which reconfirms a previous Chandra result on the northwestern part of this remna…

2017 Publications of the Astronomical Society of Japan
Suzaku 8
X-ray lags in PDS 456 revealed by Suzaku observations
DOI: 10.1093/mnras/stx2069 Bibcode: 2017MNRAS.472.1473C

Fabian, A. C.; Reynolds, C. S.; Cackett, E. M. +5 more

X-ray reverberation lags from the vicinity of supermassive black holes have been detected in almost 30 active galactic nuclei (AGNs). The soft lag, which is the time delay between the hard and soft X-ray light curves, is usually interpreted as the time difference between the direct and reflected emission, but is alternatively suggested to arise fr…

2017 Monthly Notices of the Royal Astronomical Society
Suzaku 8
Outgas analysis of mechanical cryocoolers for long lifetime
DOI: 10.1016/j.cryogenics.2017.10.001 Bibcode: 2017Cryo...88...70S

Nakagawa, Takao; Mitsuda, Kazuhisa; Kanao, Kenichi +9 more

Mechanical cryocoolers for space applications are required to have high reliability to achieve long-term operation in orbit. ASTRO-H (Hitomi), the 6th Japanese X-ray astronomy mission, has a major scientific instrument onboard-the Soft X-ray Spectrometer (SXS) with several 20K-class two-stage Stirling (2ST) coolers and a 4K-class Joule Thomson (JT…

2017 Cryogenics
Hitomi 8
Coronal X-ray emission and planetary irradiation in HD 209458
DOI: 10.1051/0004-6361/201731408 Bibcode: 2017A&A...607A.101C

Schmitt, J. H. M. M.; Czesla, S.; Salz, M. +2 more

HD 209458 is one of the benchmark objects in the study of hot Jupiter atmospheres and their evaporation through planetary winds. The expansion of the planetary atmosphere is thought to be driven by high-energy extreme ultraviolet (EUV) and X-ray irradiation. We obtained new Chandra High Resolution Camera (HRC-I) data, which unequivocally show that…

2017 Astronomy and Astrophysics
Gaia XMM-Newton 8
Tethered Prominence-CME Systems Captured during the 2012 November 13 and 2013 November 3 Total Solar Eclipses
DOI: 10.3847/2041-8213/aa9ed5 Bibcode: 2017ApJ...851L..41D

Habbal, Shadia R.; Druckmüller, Miloslav; Alzate, Nathalia +1 more

We report on white light observations of high latitude tethered prominences acquired during the total solar eclipses of 2012 November 13 and 2013 November 3, at solar maximum, with a field of view spanning several solar radii. Distinguished by their pinkish hue, characteristic of emission from neutral hydrogen and helium, the four tethered promine…

2017 The Astrophysical Journal
SOHO 8
An Improved Method for Determining the Integrated Properties of Nuclear Rings: NGC 1512
DOI: 10.3847/1538-4365/aa709e Bibcode: 2017ApJS..230...14M

Ho, Luis C.; de Grijs, Richard; Ma, Chao

The integrated properties of nuclear rings are correlated with the secular evolution and dynamics of the host galaxies of the rings, as well as with the formation and evolution of the rings’ star cluster population(s). Here we present a new method to accurately measure the spectral energy distribution and current star formation rate (SFR) of the n…

2017 The Astrophysical Journal Supplement Series
eHST 8
An Evolving GeV Spectrum from Prompt to Afterglow: The Case of GRB 160509A
DOI: 10.3847/2041-8213/aa7ca5 Bibcode: 2017ApJ...844L...7T

Tang, Qing-Wen; Wang, Xiang-Yu; Tam, Pak-Hin Thomas +1 more

We present the high-energy emission properties of GRB 160509A, from its prompt mission to late afterglow phase. GRB 160509A contains two emission episodes: 0-40 s and 280-420 s after the burst onset ({t}0). The relatively high fluence of GRB 160509A allows us to establish an evolving spectrum above 100 MeV. During the first emission epi…

2017 The Astrophysical Journal
INTEGRAL 8