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HZ Her: Stellar Radius from X-Ray Eclipse Observations, Evolutionary State, and a New Distance
DOI: 10.1088/0004-637X/793/2/79 Bibcode: 2014ApJ...793...79L

Leahy, D. A.; Abdallah, M. H.

Observations of HZ Her/Her X-1 by the Rossi X-Ray Timing Explorer (RXTE) covering high state eclipses of the neutron star are analyzed here. Models of the eclipse are used to measure the radius and atmospheric scale height of HZ Her, the stellar companion to the neutron star. The radius is 2.58-3.01 × 1011 cm, depending on system inclin…

2014 The Astrophysical Journal
eHST 41
Valles Marineris dune fields as compared with other martian populations: Diversity of dune compositions, morphologies, and thermophysical properties
DOI: 10.1016/j.icarus.2013.08.018 Bibcode: 2014Icar..230...96C

Chojnacki, Matthew; Moersch, Jeffrey E.; Burr, Devon M.

Planetary dune field properties and their bulk bedform morphologies relate to regional wind patterns, sediment supply, climate, and topography. On Mars, major occurrences of spatially contiguous low-albedo sand dunes are primarily found in three major topographic settings: impact craters, high-latitude basins, and linear troughs or valleys, the la…

2014 Icarus
MEx 41
Waves in high-speed plasmoids in the magnetosheath and at the magnetopause
DOI: 10.5194/angeo-32-991-2014 Bibcode: 2014AnGeo..32..991G

Gunell, H.; Dandouras, I.; Nilsson, H. +9 more

Plasmoids, defined here as plasma entities with a higher anti-sunward velocity component than the surrounding plasma, have been observed in the magnetosheath in recent years. During the month of March 2007 the Cluster spacecraft crossed the magnetopause near the subsolar point 13 times. Plasmoids with larger velocities than the surrounding magneto…

2014 Annales Geophysicae
Cluster 41
Directly imaging damped Lyα galaxies at z > 2 - II. Imaging and spectroscopic observations of 32 quasar fields
DOI: 10.1093/mnras/stu1512 Bibcode: 2014MNRAS.444.1282F

Prochaska, J. Xavier; Fumagalli, Michele; Kanekar, Nissim +2 more

Damped Lyα absorbers (DLAs) are a well-studied class of absorption line systems, and yet the properties of their host galaxies remain largely unknown. To investigate the origin of these systems, we have conducted an imaging survey of 32 quasar fields with intervening DLAs between z ∼ 1.9 and 3.8, leveraging a technique that allows us to image gala…

2014 Monthly Notices of the Royal Astronomical Society
eHST 41
Shockingly low water abundances in Herschel/PACS observations of low-mass protostars in Perseus
DOI: 10.1051/0004-6361/201424166 Bibcode: 2014A&A...572A...9K

Fedele, D.; van Dishoeck, E. F.; Evans, N. J. +16 more

Context. Protostars interact with their surroundings through jets and winds impinging on the envelope and creating shocks, but the nature of these shocks is still poorly understood.
Aims: Our aim is to survey far-infrared molecular line emission from a uniform and significant sample of deeply-embedded low-mass young stellar objects (YSOs) in …

2014 Astronomy and Astrophysics
Herschel 41
Temperature dependence of the sublimation rate of water ice: Influence of impurities
DOI: 10.1016/j.icarus.2014.01.025 Bibcode: 2014Icar..233..101K

Kossacki, Konrad J.; Leliwa-Kopystynski, Jacek

The sublimation rate of ice is commonly calculated using the simple Hertz-Knudsen formula. This formula is derived from the kinetic theory of gases and ignores microphysical processes determining the actual sublimation rate. The microphysical processes can be accounted for by including the temperature dependent sublimation coefficient (Kossacki, K…

2014 Icarus
Rosetta 41
Properties of Submillimeter Galaxies in the CANDELS GOODS-South Field
DOI: 10.1088/0004-637X/785/2/111 Bibcode: 2014ApJ...785..111W

Barro, Guillermo; Castellano, Marco; Ferguson, Henry C. +29 more

We derive physical properties of 10 submillimeter galaxies located in the CANDELS coverage of the GOODS-S field. The galaxies were first identified as submillimeter sources with the LABOCA bolometer and subsequently targeted for 870 µm continuum observation with ALMA. The high angular resolution of the ALMA imaging allows secure counterparts…

2014 The Astrophysical Journal
eHST 41
New Clues to the Cause of Extended Main-Sequence Turnoffs in Intermediate-age Star Clusters in the Magellanic Clouds
DOI: 10.1088/0004-637X/793/2/121 Bibcode: 2014ApJ...793..121C

Goudfrooij, Paul; Puzia, Thomas H.; Correnti, Matteo +3 more

We use the Wide Field Camera 3 on board the Hubble Space Telescope (HST) to obtain deep, high-resolution images of two intermediate-age star clusters in the Large Magellanic Cloud of relatively low mass (≈104 M ) and significantly different core radii, namely NGC 2209 and NGC 2249. For comparison purposes, we also reanalyzed…

2014 The Astrophysical Journal
eHST 41
Stellar tidal disruption candidates found by cross-correlating the ROSAT Bright Source Catalogue and XMM-Newton observations
DOI: 10.1093/mnras/stu1491 Bibcode: 2014MNRAS.444.1041K

Sazonov, S.; Khabibullin, I.

We performed a systematic search for stellar tidal disruption events (TDE) by looking for X-ray sources that were detected during the ROSAT All Sky Survey and faded by more than an order of magnitude over the next two decades according to XMM-Newton serendipitous observations. Besides a number of highly variable persistent X-ray sources (like acti…

2014 Monthly Notices of the Royal Astronomical Society
XMM-Newton 41
Magnetopause reconnection and energy conversion as influenced by the dipole tilt and the IMF Bx
DOI: 10.1002/2013JA019693 Bibcode: 2014JGRA..119.4484H

Palmroth, Minna; Hoilijoki, Sanni; Souza, Vitor M. +2 more

We study the effect of Earth's dipole tilt angle and interplanetary magnetic field (IMF) Bx and By components on the location of reconnection and the energy conversion at the magnetopause. We simulate southward IMF satisfying both inward- and outward-type Parker spiral conditions during three different dipole tilt angles usin…

2014 Journal of Geophysical Research (Space Physics)
DoubleStar 41