Search Publications

HST Imaging of the Local Volume Dwarf Galaxies Pisces A and B: Prototypes for Local Group Dwarfs
DOI: 10.3847/0004-637X/827/2/89 Bibcode: 2016ApJ...827...89T

Dolphin, Andrew E.; Weisz, Daniel R.; Putman, Mary E. +3 more

We present observations of the Pisces A and B galaxies with the Advanced Camera for Surveys on the Hubble Space Telescope. Photometry from these images clearly resolves a red giant branch (RGB) for both objects, demonstrating that they are nearby dwarf galaxies. We describe a Bayesian inferential approach to determining the distance to these galax…

2016 The Astrophysical Journal
eHST 23
Mapping Seyfert and LINER Excitation Modes in the Inner kpc of NGC 3393
DOI: 10.3847/0004-637X/829/1/46 Bibcode: 2016ApJ...829...46M

Elvis, Martin; Raymond, John; Storchi-Bergmann, Thaisa +5 more

We mapped the extended narrowline region (ENLR) of NGC 3393 on scales of r≲ 4\prime\prime (∼ 1 kpc) from the nucleus using emission line images of Hα λ6563, [O III]λ 5007, and [S II]λ λ 6717,6731, taken with the Hubble Space Telescope as part of the CHandra survey of Extended Emission line Regions in nearby Seyfert galaxies (CHEERS). By…

2016 The Astrophysical Journal
eHST 23
A statistical study on the shape and position of the magnetotail neutral sheet
DOI: 10.5194/angeo-34-303-2016 Bibcode: 2016AnGeo..34..303X

Zhang, Tielong; Nakamura, Rumi; Ge, Yasong +3 more

We study the average shape and position of the magnetotail neutral sheet based on magnetic field data obtained by Cluster, Geotail, TC-1, and THEMIS from the years 1995 to 2013. All data in the aberrated GSM (geocentric solar magnetospheric) coordinate system are normalized to the same solar wind pressure 2 nPa and downtail distance X ∼ -20RE…

2016 Annales Geophysicae
Cluster 23
Parallax of a Mira variable R Ursae Majoris studied with astrometric VLBI
DOI: 10.1093/pasj/psw069 Bibcode: 2016PASJ...68...78N

Kurayama, Tomoharu; Honma, Mareki; Nakagawa, Akiharu +5 more

We have measured an annual parallax of the Mira variable R Ursae Majoris (R UMa) with the VLBI Exploration for Radio Astronomy (VERA). From the monitoring VLBI observations over a span of about two years, we detected H2O maser spots in the LSR velocity range from 37 to 42 km s-1. We derived an annual parallax of 1.97 ± 0.05 m…

2016 Publications of the Astronomical Society of Japan
Hipparcos 23
Themis Regio, Venus: Evidence for recent (?) volcanism from VIRTIS data
DOI: 10.1016/j.icarus.2016.01.034 Bibcode: 2016Icar..271..375S

Helbert, Joern; Stofan, Ellen R.; Smrekar, Suzanne E. +1 more

Themis Regio is interpreted to be a hotspot rise underlain by one or more mantle plumes. Many volcanic features in the Themis region have high emissivity anomalies in Venus Express Visible and Infrared Thermal Imaging Spectrometer (VIRTIS) data. Other high emissivity anomalies have been found to correspond to volcanic flows interpreted to be relat…

2016 Icarus
VenusExpress 23
ALMA Imaging of the CO (6-5) Line Emission in NGC 7130*
DOI: 10.3847/0004-637X/820/2/118 Bibcode: 2016ApJ...820..118Z

Inami, Hanae; Murphy, Eric; van der Werf, Paul +11 more

In this paper, we report our high-resolution (0.″20 × 0.″14 or ∼70 × 49 pc) observations of the CO(6-5) line emission, which probes warm and dense molecular gas, and the 434 µm dust continuum in the nuclear region of NGC 7130, obtained with the Atacama Large Millimeter Array (ALMA). The CO line and dust continuum fluxes detected in our ALMA …

2016 The Astrophysical Journal
eHST 23
Magnetic Doppler imaging of the chemically peculiar star HD 125248
DOI: 10.1051/0004-6361/201527719 Bibcode: 2016A&A...588A.138R

Ilyin, I.; Ryabchikova, T.; Kochukhov, O. +1 more

Context. Intermediate-mass, chemically peculiar stars with strong magnetic fields provide an excellent opportunity to study the topology of their surface magnetic fields and the interplay between magnetic geometries and abundance inhomogeneities in the atmospheres of these stars.
Aims: We reconstruct detailed maps of the surface magnetic fiel…

2016 Astronomy and Astrophysics
IUE 23
Coronal mass ejection-related particle acceleration regions during a simple eruptive event
DOI: 10.1051/0004-6361/201528015 Bibcode: 2016A&A...590A.135S

Rouillard, Alexis P.; Klein, Karl-Ludwig; Salas-Matamoros, Carolina

An intriguing feature of many solar energetic particle (SEP) events is the detection of particles over a very extended range of longitudes in the heliosphere. This may be due to peculiarities of the magnetic field in the corona, to a broad accelerator, to cross-field transport of the particles, or to a combination of these processes. The eruptive …

2016 Astronomy and Astrophysics
SOHO 23
Constraining the physical properties of Titan's empty lake basins using nadir and off-nadir Cassini RADAR backscatter
DOI: 10.1016/j.icarus.2015.09.043 Bibcode: 2016Icar..270...57M

Zebker, H. A.; Hayes, A. G.; Malaska, M. J. +5 more

We use repeat synthetic aperture radar (SAR) observations and complementary altimetry passes acquired by the Cassini spacecraft to study the scattering properties of Titan's empty lake basins. The best-fit coefficients from fitting SAR data to a quasi-specular plus diffuse backscatter model suggest that the bright basin floors have a higher dielec…

2016 Icarus
Cassini 23
The NuSTAR view of the non-thermal emission from PSR J0437-4715
DOI: 10.1093/mnras/stw2194 Bibcode: 2016MNRAS.463.2612G

Harrison, F. A.; Boggs, S.; Stern, D. +11 more

We present a hard X-ray Nuclear Spectroscopic Telescope Array (NuSTAR) observation of PSR J0437-4715, the nearest millisecond pulsar. The known pulsations at the apparent pulse period {∼ }5.76{ ms} are observed with a significance of 3.7σ, at energies up to 20 keV above which the NuSTAR background dominates. We measure a photon index Γ = 1.50 ± 0.…

2016 Monthly Notices of the Royal Astronomical Society
XMM-Newton 23