Search Publications

High-resolution Spectroscopy of Extremely Metal-poor Stars from SDSS/SEGUE. III. Unevolved Stars with [Fe/H] ≲ -3.5
DOI: 10.3847/1538-3881/aa7a08 Bibcode: 2017AJ....154...52M

Honda, Satoshi; Beers, Timothy C.; Lee, Young Sun +2 more

We present elemental abundances for eight unevolved extremely metal-poor (EMP) stars with {T}{eff}> 5500 {{K}}, among which seven have [{Fe}/{{H}}]< -3.5. The sample is selected from the Sloan Digital Sky Survey/Sloan Extension for Galactic Understanding and Exploration (SDSS/SEGUE) and our previous high-resolution spectroscopic f…

2017 The Astronomical Journal
Gaia 33
Strong H I Lyman-α variations from an 11 Gyr-old host star: a planetary origin?
DOI: 10.1051/0004-6361/201730542 Bibcode: 2017A&A...602A.106B

Thomas, N.; Ehrenreich, D.; Lovis, C. +8 more

Kepler-444 provides a unique opportunity to probe the atmospheric composition and evolution of a compact system of exoplanets smaller than the Earth. Five planets transit this bright K star at close orbital distances, but they are too small for their putative lower atmosphere to be probed at optical/infrared wavelengths. We used the Space Telescop…

2017 Astronomy and Astrophysics
eHST 33
The Origin of the Iron-rich Knot in Tycho’s Supernova Remnant
DOI: 10.3847/1538-4357/834/2/124 Bibcode: 2017ApJ...834..124Y

Petre, Robert; Yamaguchi, Hiroya; Hughes, John P. +5 more

X-ray observations of supernova remnants (SNRs) allow us to investigate the chemical inhomogeneity of ejecta, offering unique insight into the nucleosynthesis in supernova explosions. Here we present detailed imaging and spectroscopic studies of the “Fe knot” located along the eastern rim of the Type Ia SNR Tycho (SN 1572) using Suzaku and Chandra…

2017 The Astrophysical Journal
Suzaku 33
The Impact of the Group Environment on the O VI Circumgalactic Medium
DOI: 10.3847/1538-4357/aa7743 Bibcode: 2017ApJ...844...23P

Charlton, Jane C.; Kacprzak, Glenn G.; Churchill, Christopher W. +3 more

We present a study comparing O VI λλ1031, 1037 doublet absorption found toward group galaxy environments to that of isolated galaxies. The O VI absorption in the circumgalactic medium (CGM) of isolated galaxies has been studied previously by the “Multiphase Galaxy Halos” survey, where the kinematics and absorption properties of the CGM have been i…

2017 The Astrophysical Journal
eHST 33
Doppler Shift Oscillations from a Hot Line Observed by IRIS
DOI: 10.3847/1538-4357/aa9073 Bibcode: 2017ApJ...849..113L

Huang, Y.; Li, D.; Zhang, Q. M. +4 more

We present a detailed investigation of the Doppler shift oscillations in a hot loop during an M7.1 flare on 2014 October 27 observed by the Interface Region Imaging Spectrograph. The periodic oscillations are observed in the Doppler shift of Fe xxi 1354.09 Å (log T∼ 7.05), and the dominant period is about 3.1 minutes. However, such 3.1 minute osci…

2017 The Astrophysical Journal
Hinode IRIS 33
Strongly Misaligned Triple System in SR 24 Revealed by ALMA
DOI: 10.3847/1538-4357/aa7d51 Bibcode: 2017ApJ...845...10F

Fernández-López, M.; Zapata, L. A.; Gabbasov, R.

We report the detection of the 1.3 mm continuum and the molecular emission of the disks of the young triple system SR24 by analyzing ALMA (The Atacama Large Millimeter/Submillimter Array) subarcsecond archival observations. We estimate the mass of the disks (0.025 M and 4 × 10-5 M for SR24S and SR24N, respectiv…

2017 The Astrophysical Journal
eHST 33
Luminosities and infrared excess in Type II and anomalous Cepheids in the Large and Small Magellanic Clouds
DOI: 10.1051/0004-6361/201730687 Bibcode: 2017A&A...603A..70G

Groenewegen, M. A. T.; Jurkovic, M. I.

Type II and anomalous Cepheids (ACs) are useful distance indicators when there are too few classical Cepheids or when RR Lyrae stars are too faint. Type II and ACs follow a period-luminosity relation as well, but they are less well-studied classes of objects. In this paper we study the sample of 335 Type II and ACs in the Small and Large Magellani…

2017 Astronomy and Astrophysics
AKARI 33
A swirling jet in the quasar 1308+326
DOI: 10.1051/0004-6361/201629999 Bibcode: 2017A&A...602A..29B

Britzen, S.; Krause, M.; Moser, L. +12 more

Context. Despite numerous and detailed studies of the jets of active galactic nuclei (AGN) on pc-scales, many questions are still debated. The physical nature of the jet components is one of the most prominent unsolved problems, as is the launching mechanism of jets in AGN. The quasar 1308+326 (z = 0.997) allows us to study the overall properties …

2017 Astronomy and Astrophysics
eHST 33
Noncircular features in Saturn's rings IV: Absolute radius scale and Saturn's pole direction
DOI: 10.1016/j.icarus.2017.02.007 Bibcode: 2017Icar..290...14F

Nicholson, Philip D.; French, Richard G.; McGhee-French, Colleen A. +6 more

We present a comprehensive solution for the geometry of Saturn's ring system, based on orbital fits to an extensive set of occultation observations of 122 individual ring edges and gaps. We begin with a restricted set of very high quality Cassini VIMS, UVIS, and RSS measurements for quasi-circular features in the C and B rings and the Cassini Divi…

2017 Icarus
Cassini eHST 33
VLA Measurements of Faraday Rotation through Coronal Mass Ejections
DOI: 10.1007/s11207-017-1074-7 Bibcode: 2017SoPh..292...56K

Kooi, Jason E.; Fischer, Patrick D.; Buffo, Jacob J. +1 more

Coronal mass ejections (CMEs) are large-scale eruptions of plasma from the Sun, which play an important role in space weather. Faraday rotation is the rotation of the plane of polarization that results when a linearly polarized signal passes through a magnetized plasma such as a CME. Faraday rotation is proportional to the path integral through th…

2017 Solar Physics
SOHO 33