Search Publications

High-contrast Imaging of Intermediate-mass Giants with Long-term Radial Velocity Trends
DOI: 10.3847/0004-637X/825/2/127 Bibcode: 2016ApJ...825..127R

Henning, Thomas; Terada, Hiroshi; Usuda, Tomonori +62 more

A radial velocity (RV) survey for intermediate-mass giants has been in operation for over a decade at Okayama Astrophysical Observatory (OAO). The OAO survey has revealed that some giants show long-term linear RV accelerations (RV trends), indicating the presence of outer companions. Direct-imaging observations can help clarify what objects genera…

2016 The Astrophysical Journal
eHST 12
Quantifying the Interstellar Medium and Cosmic Rays in the MBM 53, 54, and 55 Molecular Clouds and the Pegasus Loop Using Fermi-LAT Gamma-ray Observations
DOI: 10.3847/1538-4357/833/2/278 Bibcode: 2016ApJ...833..278M

Mizuno, T.; Okumura, A.; Fukui, Y. +4 more

A study of the interstellar medium (ISM) and cosmic rays (CRs) using Fermi Large Area Telescope (LAT) data, in a region encompassing the nearby molecular clouds MBM 53, 54, and 55 and a far-infrared loop-like structure in Pegasus, is reported. By comparing the Planck dust thermal emission model with Fermi-LAT γ-ray data, it was found that neither …

2016 The Astrophysical Journal
Planck 12
Comparison of CME/Shock Propagation Models with Heliospheric Imaging and In Situ Observations
DOI: 10.3847/0004-637X/830/1/48 Bibcode: 2016ApJ...830...48Z

Lu, Lei; Feng, Xueshang; Liu, Ying D. +3 more

The prediction of the arrival time for fast coronal mass ejections (CMEs) and their associated shocks is highly desirable in space weather studies. In this paper, we use two shock propagation models, I.e., Data Guided Shock Time Of Arrival (DGSTOA) and Data Guided Shock Propagation Model (DGSPM), to predict the kinematical evolution of interplanet…

2016 The Astrophysical Journal
SOHO 12
Tracing back the evolution of the candidate LBV HD 168625
DOI: 10.1051/0004-6361/201628584 Bibcode: 2016A&A...594A..94M

Mahy, L.; Waelkens, C.; Royer, P. +1 more

Context. The luminous blue variable phase is a crucial transitory phase that is not clearly understood in the massive star evolution.
Aims: We have obtained far-infrared Herschel/PACS imaging and spectroscopic observations of the nebula surrounding the candidate LBV HD 168625. By combining these data with optical spectra of the central star, …

2016 Astronomy and Astrophysics
Herschel 12
The Comparison of Total Electron Content Between Radio and Thompson Scattering
DOI: 10.1007/s11207-015-0834-5 Bibcode: 2016SoPh..291..465J

Llebaria, A.; Lamy, P.; Jensen, E. A. +5 more

The total electron content (TEC) of the solar corona in June 2002 is calculated by three observational techniques and the results are compared. The first technique is solar rotational tomography (SRT) applied to a 14-day time series of LASCO-C2 polarized brightness images, and the other two techniques use the Cassini spacecraft radio beacon for Do…

2016 Solar Physics
SOHO 12
Properties of Interstellar Medium In Infrared-bright QSOs Probed by [O I] 63 um and [C II] 158 um Emission Lines
DOI: 10.3847/0004-637X/824/2/146 Bibcode: 2016ApJ...824..146Z

Tsai, Chao-Wei; Zhao, Yinghe; Yan, Lin

We present a study of the interstellar medium (ISM) in the host galaxies of nine QSOs at 0.1 < z < 0.2 with black hole masses of 3× {10}7 {M} to 3× {10}9 {M} based on the far-IR spectroscopy taken with Herschel Space Observatory. We detect the [O I] 63 µm ([C II] 158 µm) emission in…

2016 The Astrophysical Journal
Herschel 12
Search for Gamma-Ray Emission from AE Aquarii with Seven Years of Fermi-LAT Observations
DOI: 10.3847/0004-637X/832/1/35 Bibcode: 2016ApJ...832...35L

Rea, Nanda; Torres, Diego F.; Li, Jian +4 more

AE Aquarii (AE Aqr) is a cataclysmic binary hosting one of the fastest rotating ({P}{spin} = 33.08 s) white dwarfs (WDs) known. Based on seven years of Fermi Large Area Telescope (LAT) Pass 8 data, we report on a deep search for gamma-ray emission from AE Aqr. Using X-ray observations from ASCA, XMM-Newton, Chandra, Swift, Suzaku, and N…

2016 The Astrophysical Journal
Suzaku XMM-Newton 12
The ACS LCID Project. XI. On the Early Time Resolution of SFHs of Local Group Dwarf Galaxies: Comparing the Effects of Reionization in Models with Observations
DOI: 10.3847/0004-637X/823/1/9 Bibcode: 2016ApJ...823....9A

Dolphin, Andrew; Skillman, Evan; Monelli, Matteo +10 more

The analysis of the early star formation history (SFH) of nearby galaxies, obtained from their resolved stellar populations, is relevant as a test for cosmological models. However, the early time resolution of observationally derived SFHs is limited by several factors. Thus, direct comparison of observationally derived SFHs with those derived from…

2016 The Astrophysical Journal
eHST 12
Stratigraphy and formation of clays, sulfates, and hydrated silica within a depression in Coprates Catena, Mars
DOI: 10.1002/2015JE004954 Bibcode: 2016JGRE..121..805W

Weitz, Catherine M.; Bishop, Janice L.

We investigate the morphology, mineralogy, and stratigraphy of light-toned layered deposits within a trough of Coprates Catena, centered at -15°N, 300°E. One of the deposits in the eastern portion of the trough contains numerous hydrated minerals, including Al-phyllosilicates, Fe/Mg-phyllosilicates, hydrated silica, hydrated sulfates, jarosite and…

2016 Journal of Geophysical Research (Planets)
MEx 12
Cosmological Parameters from CMB Maps without Likelihood Approximation
DOI: 10.3847/0004-637X/820/1/31 Bibcode: 2016ApJ...820...31R

Eriksen, H. K.; Wehus, I. K.; Racine, B. +1 more

We propose an efficient Bayesian Markov chain Monte Carlo (MCMC) algorithm for estimating cosmological parameters from cosmic microwave background (CMB) data without the use of likelihood approximations. It builds on a previously developed Gibbs sampling framework that allows for exploration of the joint CMB sky signal and power spectrum posterior…

2016 The Astrophysical Journal
Planck 12