Search Publications

Carbon Abundances in Starburst Galaxies of the Local Universe
DOI: 10.3847/1538-4357/aa88bf Bibcode: 2017ApJ...847..107P

Leitherer, Claus; Wofford, Aida; Kewley, Lisa +2 more

The cosmological origin of carbon, the fourth most abundant element in the universe, is not well known and a matter of heavy debate. We investigate the behavior of C/O to O/H in order to constrain the production mechanism of carbon. We measured emission-line intensities in the spectral range from 1600 to 10000 Å on Space Telescope Imaging Spectrog…

2017 The Astrophysical Journal
eHST 16
Search for the warm-hot intergalactic medium around A 2744 using Suzaku
DOI: 10.1093/pasj/psx011 Bibcode: 2017PASJ...69...39H

Finoguenov, Alexis; Akamatsu, Hiroki; Ota, Naomi +2 more

We present the results from Suzaku satellite observations of the surrounding region of a galaxy cluster, A 2744, at z = 0.3. To search for oxygen emission lines from the warm-hot intergalactic medium (WHIM), we analyzed X-ray spectra from two northeastern regions 2.2-3.3 and 3.3-4.4 Mpc from the center of the cluster, which offers the first test o…

2017 Publications of the Astronomical Society of Japan
Suzaku XMM-Newton 16
VLBA Trigonometric Parallax Measurement of the Semi-regular Variable RT Vir
DOI: 10.3847/1538-4357/aa8ee9 Bibcode: 2017ApJ...849...99Z

Menten, Karl M.; Honma, Mareki; Reid, Mark J. +4 more

We report a trigonometric parallax measurement of 22 GHz H2O masers toward the semi-regular variable RT Vir from multi-epoch Very Long Baseline Array observations. The parallax of 4.417 ± 0.134 mas, corresponding to a distance of 226 ± 7 pc, is significantly different from the Hipparcos parallax, but is consistent with a distance derive…

2017 The Astrophysical Journal
Gaia Hipparcos 16
What is the Milky Way outer halo made of?. High resolution spectroscopy of distant red giants
DOI: 10.1051/0004-6361/201731879 Bibcode: 2017A&A...608A.145B

Minniti, D.; Jablonka, P.; Starkenburg, E. +5 more

In a framework where galaxies form hierarchically, extended stellar haloes are predicted to be an ubiquitous feature around Milky Way-like galaxies and to consist mainly of the shredded stellar component of smaller galactic systems. The type of accreted stellar systems are expected to vary according to the specific accretion and merging history of…

2017 Astronomy and Astrophysics
Gaia 16
Measurement of dust optical depth using the solar irradiance sensor (SIS) onboard the ExoMars 2016 EDM
DOI: 10.1016/j.pss.2017.01.015 Bibcode: 2017P&SS..138...33T

Rannou, P.; Toledo, D.; Gómez, L. +5 more

The solar irradiance sensor (SIS) was included in the DREAMS package onboard the ExoMars 2016 Entry Descent and Landing Demonstrator Module, and has been selected in the METEO meteorological station onboard the ExoMars 2020 Lander. This instrument is designed to measure at different time intervals the scattered flux or the sum of direct flux and s…

2017 Planetary and Space Science
ExoMars-16 16
Discovery of an H I-rich Gas Reservoir in the Outskirts of SZ-effect-selected Clusters
DOI: 10.3847/2041-8213/aa8559 Bibcode: 2017ApJ...846L...8M

Nagai, Daisuke; Schaye, Joop; Muzahid, Sowgat +2 more

We report on the detection of three strong H I absorbers originating in the outskirts (I.e., impact parameter, {ρ }{cl} ≈ (1.6-4.7)r 500) of three massive ({M}500∼ 3× {10}14 M ) clusters of galaxies at redshift {z}{cl}≈ 0.46, in the Hubble Space Telescope Cosmic Origins Spectrograp…

2017 The Astrophysical Journal
eHST 16
Observations of Lyα and O VI: Signatures of Cooling and Star Formation in a Massive Central Cluster Galaxy
DOI: 10.3847/1538-4357/835/2/216 Bibcode: 2017ApJ...835..216D

Donahue, Megan; Voit, G. Mark; Connor, Thomas +1 more

We report new Hubble Space Telescope COS and Space Telescope Imaging Spectrograph spectroscopy of a star-forming region (∼ 100 {M} yr-1) in the center of the X-ray cluster RX J1532.9+3021 (z = 0.362), to follow-up the CLASH team discovery of luminous UV filaments and knots in the central massive galaxy. We detect broad (∼50…

2017 The Astrophysical Journal
eHST 16
Interchange Reconnection Associated with a Confined Filament Eruption: Implications for the Source of Transient Cold-dense Plasma in Solar Winds
DOI: 10.3847/1538-4357/aa6b03 Bibcode: 2017ApJ...840....3Z

Li, Gang; Chen, Yao; Zheng, Ruisheng +2 more

The cold-dense plasma is occasionally detected in the solar wind with in situ data, but the source of the cold-dense plasma remains illusive. Interchange reconnections (IRs) between closed fields and nearby open fields are known to contribute to the formation of solar winds. We present a confined filament eruption associated with a puff-like coron…

2017 The Astrophysical Journal
SOHO 16
Bidirectional reflectance of laboratory cometary analogues to interpret the spectrophotometric properties of the nucleus of comet 67P/Churyumov-Gerasimenko
DOI: 10.1016/j.pss.2017.09.009 Bibcode: 2017P&SS..148....1J

Thomas, Nicolas; Fornasier, Sonia; Pommerol, Antoine +5 more

In this work we provide measurements of the bidirectional reflectance in the VIS-NIR spectral range for a selection of laboratory samples to deduce parameters such as their visible spectrum, phase curve, hemispheric albedo and phase reddening. The aim is to simulate the reflectance of the comet nucleus in order to aid the interpretation of data fr…

2017 Planetary and Space Science
Rosetta 16
Cometary coma dust size distribution from in situ IR spectra
DOI: 10.1093/mnras/stx1873 Bibcode: 2017MNRAS.469S.598R

Fulle, M.; Mottola, S.; D'Aversa, E. +16 more

Dust is the most abundant component in cometary comae. Here, we investigate the dust size distribution in 67P/Churyumov-Gerasimenko (67P/CG) using data from the Rosetta spacecraft that was in close proximity to the comet from 2014 August to 2016 September. The Visual, Infrared and Thermal Imaging Spectrometer (VIRTIS-M), spectral range of 0.25-5 &…

2017 Monthly Notices of the Royal Astronomical Society
Rosetta 16