Search Publications

Non-Maxwellian Analysis of the Transition-region Line Profiles Observed by the Interface Region Imaging Spectrograph
DOI: 10.3847/1538-4357/aa71a8 Bibcode: 2017ApJ...842...19D

Polito, Vanessa; Del Zanna, Giulio; Testa, Paola +2 more

We investigate the nature of the spectral line profiles for transition-region (TR) ions observed with the Interface Region Imaging Spectrograph (IRIS). In this context, we analyzed an active-region observation performed by IRIS in its 1400 Å spectral window. The TR lines are found to exhibit significant wings in their spectral profiles, which can …

2017 The Astrophysical Journal
IRIS 39
Cloud Structure of Three Galactic Infrared Dark Star-forming Regions from Combining Ground- and Space-based Bolometric Observations
DOI: 10.3847/1538-4357/aa6c67 Bibcode: 2017ApJ...840...22L

Li, Di; Qian, Lei; Ginsburg, Adam +12 more

We have modified the iterative procedure introduced by Lin et al., to systematically combine the submillimeter images taken from ground-based (e.g., CSO, JCMT, APEX) and space (e.g., Herschel, Planck) telescopes. We applied the updated procedure to observations of three well-studied Infrared Dark Clouds (IRDCs): G11.11-0.12, G14.225-0.506, and G28…

2017 The Astrophysical Journal
Herschel Planck 39
Line Ratios for Solar Wind Charge Exchange with Comets
DOI: 10.3847/1538-4357/aa7752 Bibcode: 2017ApJ...844....7M

Gu, L.; Kaastra, J.; Shelton, R. L. +4 more

Charge exchange (CX) has emerged in X-ray emission modeling as a significant process that must be considered in many astrophysical environments—particularly comets. Comets host an interaction between solar wind ions and cometary neutrals to promote solar wind charge exchange (SWCX). X-ray observatories provide astronomers and astrophysicists with …

2017 The Astrophysical Journal
XMM-Newton 39
High-resolution Statistics of Solar Wind Turbulence at Kinetic Scales Using the Magnetospheric Multiscale Mission
DOI: 10.3847/2041-8213/aa7ddd Bibcode: 2017ApJ...844L...9C

Russell, C. T.; Fuselier, S. A.; Torbert, R. B. +10 more

Using data from the Magnetospheric Multiscale (MMS) and Cluster missions obtained in the solar wind, we examine second-order and fourth-order structure functions at varying spatial lags normalized to ion inertial scales. The analysis includes direct two-spacecraft results and single-spacecraft results employing the familiar Taylor frozen-in flow a…

2017 The Astrophysical Journal
Cluster 39
ALMA Pinpoints a Strong Overdensity of U/LIRGs in the Massive Cluster XCS J2215 at z = 1.46
DOI: 10.3847/1538-4357/aa93f6 Bibcode: 2017ApJ...849..154S

Smail, Ian; Hilton, Matt; Swinbank, A. M. +3 more

We surveyed the core regions of the z = 1.46 cluster XCS J2215.9-1738 with the Atacama Large Millimeter Array (ALMA) and the MUSE-GALACSI spectrograph on the Very Large Telescope (VLT). We obtained high spatial resolution observations with ALMA of the 1.2 mm dust continuum and molecular gas emission in the central regions of the cluster. These obs…

2017 The Astrophysical Journal
eHST 39
Observational Evidence for High Neutronization in Supernova Remnants: Implications for Type Ia Supernova Progenitors
DOI: 10.3847/1538-4357/aa72f8 Bibcode: 2017ApJ...843...35M

Mori, Hideyuki; Yamaguchi, Hiroya; Badenes, Carles +8 more

The physical process whereby a carbon-oxygen white dwarf explodes as a Type Ia supernova (SN Ia) remains highly uncertain. The degree of neutronization in SN Ia ejecta holds clues to this process because it depends on the mass and the metallicity of the stellar progenitor, and on the thermodynamic history prior to the explosion. We report on a new…

2017 The Astrophysical Journal
Suzaku 39
Gas Sloshing Regulates and Records the Evolution of the Fornax Cluster
DOI: 10.3847/1538-4357/aa989e Bibcode: 2017ApJ...851...69S

Jones, Christine; Nulsen, Paul E. J.; Kraft, Ralph P. +7 more

We present results of a joint Chandra and XMM-Newton analysis of the Fornax Cluster, the nearest galaxy cluster in the southern sky. Signatures of merger-induced gas sloshing can be seen in the X-ray image. We identify four sloshing cold fronts in the intracluster medium, residing at radii of 3 kpc (west), 10 kpc (northeast), 30 kpc (southwest), a…

2017 The Astrophysical Journal
XMM-Newton 39
Dust Abundance Variations in the Magellanic Clouds: Probing the Life-cycle of Metals with All-sky Surveys
DOI: 10.3847/1538-4357/aa7067 Bibcode: 2017ApJ...841...72R

Bot, Caroline; Roman-Duval, Julia; Gordon, Karl +1 more

Observations and modeling suggest that dust abundance (gas-to-dust ratio, G/D) depends on (surface) density. Variations of the G/D provide timescale constraints for the different processes involved in the life cycle of metals in galaxies. Recent G/D measurements based on Herschel data suggest a factor of 5-10 decrease in dust abundance between the…

2017 The Astrophysical Journal
Planck 39
The HDUV Survey: Six Lyman Continuum Emitter Candidates at z ∼ 2 Revealed by HST UV Imaging
DOI: 10.3847/1538-4357/aa8863 Bibcode: 2017ApJ...847...12N

Oesch, P. A.; Carollo, C. M.; Nelson, E. J. +14 more

We present six galaxies at z∼ 2 that show evidence of Lyman continuum (LyC) emission based on the newly acquired UV imaging of the Hubble Deep UV legacy survey (HDUV) conducted with the WFC3/UVIS camera on the Hubble Space Telescope (HST). At the redshift of these sources, the HDUV F275W images partially probe the ionizing continuum. By exploiting…

2017 The Astrophysical Journal
eHST 39
Formation of Methylamine and Ethylamine in Extraterrestrial Ices and Their Role as Fundamental Building Blocks of Proteinogenic α-amino Acids
DOI: 10.3847/1538-4357/aa7edd Bibcode: 2017ApJ...845...83F

Kaiser, Ralf I.; Förstel, Marko; Bergantini, Alexandre +2 more

The -CH-NH2 moiety represents the fundamental building block of all proteinogenic amino acids, with the cyclic amino acid proline being a special case (-CH-NH- in proline). Exploiting a chemical retrosynthesis, we reveal that methylamine (CH3NH2) and/or ethylamine (CH3CH2NH2) are es…

2017 The Astrophysical Journal
Rosetta 38