Search Publications

Navy Precision Optical Interferometer Measurements of 10 Stellar Oscillators
DOI: 10.1088/0004-637X/781/2/90 Bibcode: 2014ApJ...781...90B

van Belle, Gerard T.; Zavala, R. T.; Schmitt, Henrique R. +3 more

Using the Navy Precision Optical Interferometer, we measured the angular diameters of 10 stars that have previously measured solar-like oscillations. Our sample covered a range of evolutionary stages but focused on evolved subgiant and giant stars. We combined our angular diameters with Hipparcos parallaxes to determine the stars' physical radii, …

2014 The Astrophysical Journal
Hipparcos 25
RX J0848.6+4453: The Evolution of Galaxy Sizes and Stellar Populations in a z = 1.27 Cluster
DOI: 10.1088/0004-6256/148/6/117 Bibcode: 2014AJ....148..117J

Toft, Sune; Jørgensen, Inger; Chiboucas, Kristin +4 more

RX J0848.6+4453 (Lynx W) at redshift 1.27 is part of the Lynx Supercluster of galaxies. We present an analysis of the stellar populations and star formation history for a sample of 24 members of the cluster. Our study is based on deep optical spectroscopy obtained with Gemini North combined with imaging data from Hubble Space Telescope. Focusing o…

2014 The Astronomical Journal
eHST 25
Abundances in the ejecta of core-collapse supernova remnants G350.1-0.3 and G349.7+0.2
DOI: 10.1093/pasj/psu043 Bibcode: 2014PASJ...66...68Y

Koyama, Katsuji; Uchida, Hiroyuki; Yasumi, Masato +5 more

We present Suzaku results of the two Galactic supernova remnants (SNRs) G350.1-0.3 and G349.7+0.2. We find Al and Ni Kα lines from both the SNRs for the first time, in addition to previously detected K-shell lines of Mg, Si, S, Ar, Ca, and Fe. The spectra are well described by two optically thin thermal plasmas: a low-temperature (low-kT) plasma i…

2014 Publications of the Astronomical Society of Japan
Suzaku 25
Herschel observations of debris discs orbiting planet-hosting subgiants
DOI: 10.1093/mnras/stt2128 Bibcode: 2014MNRAS.437.3288B

Wyatt, Mark C.; Johnson, John A.; Kennedy, Grant M. +2 more

Debris discs are commonly detected orbiting main-sequence stars, yet little is known regarding their fate as the star evolves to become a giant. Recent observations of radial velocity detected planets orbiting giant stars highlight this population and its importance for probing, for example, the population of planetary systems orbiting intermediat…

2014 Monthly Notices of the Royal Astronomical Society
Herschel 25
The long-period Galactic Cepheid RS Puppis. III. A geometric distance from HST polarimetric imaging of its light echoes
DOI: 10.1051/0004-6361/201424395 Bibcode: 2014A&A...572A...7K

Szabados, L.; Kervella, P.; Anderson, R. I. +8 more

As one of the most luminous Cepheids in the Milky Way, the 41.5-day RS Puppis is an analog of the long-period Cepheids used to measure extragalactic distances. An accurate distance to this star would therefore help anchor the zero-point of the bright end of the period-luminosity relation. But, at a distance of about 2 kpc, RS Pup is too far away f…

2014 Astronomy and Astrophysics
eHST 25
Physical structure of the photodissociation regions in NGC 7023. Observations of gas and dust emission with Herschel
DOI: 10.1051/0004-6361/201322711 Bibcode: 2014A&A...569A.109K

Abergel, A.; Teyssier, D.; Zavagno, A. +16 more

Context. The determination of the physical conditions in molecular clouds is a key step towards our understanding of their formation and evolution of associated star formation. We investigate the density, temperature, and column density of both dust and gas in the photodissociation regions (PDRs) located at the interface between the atomic and col…

2014 Astronomy and Astrophysics
Herschel 25
Proton acceleration at two-dimensional dipolarization fronts in the magnetotail
DOI: 10.1002/2014JA020421 Bibcode: 2014JGRA..119.8929G

Artemyev, A.; Zimbardo, G.; Greco, A.

Transient reconnection events in the planetary magnetotail give rise to fast plasma jets, whose leading edges are called dipolarization fronts. We perform a test particle simulation of ion acceleration in a 2-D model of dipolarization fronts. We study the dependence of acceleration on several parameters of the model. We obtain that the interaction…

2014 Journal of Geophysical Research (Space Physics)
Cluster 25
Heavy metals in a light white dwarf: abundances of the metal-rich, extremely low-mass GALEX J1717+6757
DOI: 10.1093/mnras/stu1518 Bibcode: 2014MNRAS.444.1674H

Hermes, J. J.; Gänsicke, B. T.; Dhillon, V. S. +9 more

Using the Hubble Space Telescope, we detail the first abundance analysis enabled by far-ultraviolet spectroscopy of a low-mass (≃0.19 M) white dwarf (WD), GALEX J1717+6757, which is in a 5.9-h binary with a fainter, more-massive companion. We see absorption from nine metals, including roughly solar abundances of Ca, Fe, Ti, and P. We d…

2014 Monthly Notices of the Royal Astronomical Society
eHST 25
The Chemical Evolution of Phosphorus
DOI: 10.1088/2041-8205/796/2/L24 Bibcode: 2014ApJ...796L..24J

Matteucci, Francesca; Roederer, Ian U.; Frebel, Anna +3 more

Phosphorus is one of the few remaining light elements for which little is known about its nucleosynthetic origin and chemical evolution, given the lack of optical absorption lines in the spectra of long-lived FGK-type stars. We have identified a P I doublet in the near-ultraviolet (2135/2136 Å) that is measurable in stars of low metallicity. Using…

2014 The Astrophysical Journal
eHST 25
Temporal Evolution of Solar Wind Ion Composition and their Source Coronal Holes during the Declining Phase of Cycle 23. I. Low-latitude Extension of Polar Coronal Holes
DOI: 10.1088/0004-637X/787/2/121 Bibcode: 2014ApJ...787..121K

Young, Peter R.; Wang, Yi-Ming; Ko, Yuan-Kuen +2 more

We analyzed 27 solar wind (SW) intervals during the declining phase of cycle 23, whose source coronal holes (CHs) can be unambiguously identified and are associated with one of the polar CHs. We found that the SW ions have a temporal trend of decreasing ionization state, and such a trend is different between the slow and fast SW. The photospheric …

2014 The Astrophysical Journal
SOHO 25