Search Publications

A robust measurement of the mass outflow rate of the galactic outflow from NGC 6090
DOI: 10.1093/mnras/stw1951 Bibcode: 2016MNRAS.463..541C

Chisholm, John; Leitherer, Claus; Tremonti Christy, A. +1 more

To evaluate the impact of stellar feedback, it is critical to estimate the mass outflow rates of galaxies. Past estimates have been plagued by uncertain assumptions about the outflow geometry, metallicity, and ionization fraction. Here we use Hubble Space Telescope ultraviolet spectroscopic observations of the nearby starburst NGC 6090 to demonstr…

2016 Monthly Notices of the Royal Astronomical Society
eHST 56
Catalog of equatorial coordinates and B-magnitudes of stars of the FON project
DOI: 10.3103/S0884591316050032 Bibcode: 2016KPCB...32..260A

Andruk, V. M.; Pakuliak, L. K.; Golovnia, V. V. +4 more

The catalog of equatorial coordinates α and δ and B-magnitudes of stars of the northern sky (from–4° to +90°) was created as a part of the FON project at the Main Astronomical Observatory of the National Academy of Sciences of Ukraine. The data accumulated in the Joint Digital Archive of the Ukrainian Virtual Observatory were used. The total numbe…

2016 Kinematics and Physics of Celestial Bodies
Hipparcos 56
Determining Ages of APOGEE Giants with Known Distances
DOI: 10.3847/0004-637X/817/1/40 Bibcode: 2016ApJ...817...40F

Bovy, Jo; Majewski, Steven R.; Feuillet, Diane K. +4 more

We present a sample of 705 local giant stars observed using the New Mexico State University 1 m telescope with the Sloan Digital Sky Survey-III/Apache Point Observatory Galactic Evolution Experiment (APOGEE) spectrograph, for which we estimate stellar ages and the local star formation history (SFH). The high-resolution (R ∼ 22,500), near infrared …

2016 The Astrophysical Journal
Hipparcos 56
Tracing extended low-velocity shocks through SiO emission. Case study of the W43-MM1 ridge
DOI: 10.1051/0004-6361/201629077 Bibcode: 2016A&A...595A.122L

Hill, T.; Schneider, N.; Maury, A. +8 more


Aims: Previous literature suggests that the densest structures in the interstellar medium form through colliding flows, but patent evidence of this process is still missing. Recent literature proposes using SiO line emission to trace low-velocity shocks associated with cloud formation through collision. In this paper we investigate the bright…

2016 Astronomy and Astrophysics
Herschel 56
Density diagnostics derived from the O iv and S iv intercombination lines observed by IRIS
DOI: 10.1051/0004-6361/201628965 Bibcode: 2016A&A...594A..64P

Mason, H. E.; Del Zanna, G.; Reeves, K. K. +3 more

The intensity of the O iv 2s2 2p 2P-2s2p24P and S iv 3 s2 3p 2P-3s 3p24 P intercombination lines around 1400 Å observed with the Interface Region Imaging Spectrograph (IRIS) provide a useful tool to diagnose the electron number density (Ne) in the so…

2016 Astronomy and Astrophysics
IRIS 56
CSI 2264: Characterizing Young Stars in NGC 2264 with Stochastically Varying Light Curves
DOI: 10.3847/0004-6256/151/3/60 Bibcode: 2016AJ....151...60S

Song, Inseok; Gillen, Edward; Cody, Ann Marie +25 more

We provide CoRoT and Spitzer light curves and other supporting data for 17 classical T Tauri stars in NGC 2264 whose CoRoT light curves exemplify the “stochastic” light curve class as defined in 2014 by Cody et al. The most probable physical mechanism to explain the optical variability within this light curve class is time-dependent mass accretion…

2016 The Astronomical Journal
CoRoT 55
Cosmochemical implications of CONSERT permittivity characterization of 67P/CG
DOI: 10.1093/mnras/stx040 Bibcode: 2016MNRAS.462S.516H

Lasue, J.; Quirico, E.; Kofman, W. +7 more

Analysis of the propagation of the Comet Nucleus Sounding Experiment by Radiowave Transmission (CONSERT) signal throughout the small lobe of the 67P/CG nucleus has permitted us to deduce the real part of the permittivity, at a value of 1.27 ± 0.05. The first interpretation of this value, using the dielectric properties of mixtures of ices (H2…

2016 Monthly Notices of the Royal Astronomical Society
Rosetta 55
Cross-scale energy transport in space plasmas
DOI: 10.1038/nphys3869 Bibcode: 2016NatPh..12.1164M

Nykyri, K.; Moore, T. W.; Dimmock, A. P.

The solar wind is a supersonic magnetized plasma streaming far into the heliosphere. Although cooling as it flows, it is rapidly heated upon encountering planetary obstacles. At Earth, this interaction forms the magnetosphere and its sub-regions. The present paper focuses on particle heating across the boundary separating the shocked solar wind an…

2016 Nature Physics
Cluster 55
Fan-shaped jets above the light bridge of a sunspot driven by reconnection
DOI: 10.1051/0004-6361/201528022 Bibcode: 2016A&A...590A..57R

Rouppe van der Voort, Luc; Leenaarts, Jorrit; Robustini, Carolina +1 more

We report on a fan-shaped set of high-speed jets above a strongly magnetized light bridge (LB) of a sunspot observed in the Hα line. We study the origin, dynamics, and thermal properties of the jets using high-resolution imaging spectroscopy in Hα from the Swedish 1m Solar Telescope and data from the Solar Dynamics Observatory and Hinode. The Hα j…

2016 Astronomy and Astrophysics
Hinode 55
SN Refsdal: Classification as a Luminous and Blue SN 1987A-like Type II Supernova
DOI: 10.3847/0004-637X/831/2/205 Bibcode: 2016ApJ...831..205K

Zitrin, A.; Filippenko, A. V.; Foley, R. J. +20 more

We have acquired Hubble Space Telescope (HST) and Very Large Telescope near-infrared spectra and images of supernova (SN) Refsdal after its discovery as an Einstein cross in fall 2014. The HST light curve of SN Refsdal has a shape consistent with the distinctive, slowly rising light curves of SN 1987A-like SNe, and we find strong evidence for a br…

2016 The Astrophysical Journal
eHST 55