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Imaging a Central Ionized Component, a Narrow Ring, and the CO Snowline in the Multigapped Disk of HD 169142
DOI: 10.3847/1538-4357/aa6620 Bibcode: 2017ApJ...838...97M

Carrasco-González, Carlos; Rodríguez, Luis F.; Macías, Enrique +5 more

We report Very Large Array observations at 7 mm, 9 mm, and 3 cm toward the pre-transitional disk of the Herbig Ae star HD 169142. These observations have allowed us to study the millimeter emission of this disk with the highest angular resolution so far (0.″12 × 0.″09, or 14 au × 11 au, at 7 mm). Our 7 and 9 mm images show a narrow ring of emissio…

2017 The Astrophysical Journal
Gaia 39
The Interstellar Medium in High-redshift Submillimeter Galaxies as Probed by Infrared Spectroscopy*
DOI: 10.3847/1538-4357/837/1/12 Bibcode: 2017ApJ...837...12W

Smith, Matthew W. L.; van der Werf, Paul; Valtchanov, Ivan +21 more

Submillimeter galaxies (SMGs) at z≳ 1 are luminous in the far-infrared, and have star formation rates, SFR, of hundreds to thousands of solar masses per year. However, it is unclear whether they are true analogs of local ULIRGs or whether the mode of their star formation is more similar to that in local disk galaxies. We target these questions by …

2017 The Astrophysical Journal
Herschel 39
First Detection of Prominence Material Embedded within a 2 × 106 K CME Front Streaming away at 100-1500 km s-1 in the Solar Corona
DOI: 10.3847/2041-8213/aa7460 Bibcode: 2017ApJ...842L...7D

Habbal, Shadia Rifai; Ding, Adalbert

Coronal mass ejections (CMEs) are the largest and most dynamic explosions detected in the million degree solar corona, with speeds reaching up to 3000 km s-1 at Earth’s orbit. Triggered by the eruption of prominences, in most cases, one of the outstanding questions pertaining to the dynamic CME-prominence system is the fate of the cool …

2017 The Astrophysical Journal
SOHO 39
DHIGLS: DRAO H I Intermediate Galactic Latitude Survey
DOI: 10.3847/1538-4357/834/2/126 Bibcode: 2017ApJ...834..126B

Martin, P. G.; Kothes, R.; Lockman, Felix J. +5 more

Observations of Galactic H I gas for seven targeted regions at intermediate Galactic latitude are presented at 1\prime angular resolution using data from the DRAO Synthesis Telescope (ST) and the Green Bank Telescope (GBT). The DHIGLS data are the most extensive arcminute-resolution measurements of the diffuse atomic interstellar medium…

2017 The Astrophysical Journal
Planck 39
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