Search Publications

On the Origin of the Flare Emission in IRIS’ SJI 2832 Filter:Balmer Continuum or Spectral Lines?
DOI: 10.3847/1538-4357/aa62fe Bibcode: 2017ApJ...837..160K

Krucker, Säm; Heinzel, Petr; Kleint, Lucia

Continuum (“white-light,” WL) emission dominates the energetics of flares. Filter-based observations, such as the IRIS SJI 2832 filter, show WL-like brightenings during flares, but it is unclear whether the emission arises from real continuum emission or enhanced spectral lines, possibly turning into emission. The difficulty in filter-based observ…

2017 The Astrophysical Journal
IRIS 21
Separating galaxies from the cluster dark matter halo in Abell 611
DOI: 10.1093/mnras/stw3048 Bibcode: 2017MNRAS.465.4589M

Zitrin, A.; Koekemoer, A.; Postman, M. +7 more

We investigate the mass content of galaxies in the core of the galaxy cluster Abell 611. We perform a strong lensing analysis of the cluster core and use velocity dispersion measurements for individual cluster members as additional constraints. Despite the small number of multiply-imaged systems and cluster members with central velocity dispersion…

2017 Monthly Notices of the Royal Astronomical Society
eHST 21
No Sign of Strong Molecular Gas Outflow in an Infrared-bright Dust-obscured Galaxy with Strong Ionized-gas Outflow
DOI: 10.3847/1538-4357/aa9d17 Bibcode: 2017ApJ...851...98T

Imanishi, Masatoshi; Toba, Yoshiki; Nagao, Tohru +4 more

We report the discovery of an infrared (IR)-bright dust-obscured galaxy (DOG) that shows a strong ionized-gas outflow but no significant molecular gas outflow. Based on detailed analysis of their optical spectra, we found some peculiar IR-bright DOGs that show strong ionized-gas outflow ([O III] λ5007) from the central active galactic nucleus (AGN…

2017 The Astrophysical Journal
AKARI 21
Exploratory Spectroscopy of Magnetic Cataclysmic Variables Candidates and Other Variable Objects
DOI: 10.3847/1538-3881/aa610d Bibcode: 2017AJ....153..144O

Oliveira, A. S.; Rodrigues, C. V.; Palhares, M. S. +5 more

The increasing number of synoptic surveys made by small robotic telescopes, such as the photometric Catalina Real-Time Transient Survey (CRTS), provides a unique opportunity to discover variable sources and improves the statistical samples of such classes of objects. Our goal is the discovery of magnetic Cataclysmic Variables (mCVs). These are rar…

2017 The Astronomical Journal
XMM-Newton 21
The Not So Simple Globular Cluster ω Cen. I. Spatial Distribution of the Multiple Stellar Populations
DOI: 10.3847/1538-3881/aa6397 Bibcode: 2017AJ....153..175C

Rest, A.; Zenteno, A.; Saha, A. +8 more

We present a multi-band photometric catalog of ≈1.7 million cluster members for a field of view of ≈2° × 2° across ω Cen. Photometry is based on images collected with the Dark Energy Camera on the 4 m Blanco telescope and the Advanced Camera for Surveys on the Hubble Space Telescope. The unprecedented photometric accuracy and field coverage allowe…

2017 The Astronomical Journal
eHST 21
Ion hole formation and nonlinear generation of electromagnetic ion cyclotron waves: THEMIS observations
DOI: 10.1002/2017GL074254 Bibcode: 2017GeoRL..44.8730S

Miyoshi, Yoshizumi; Kasahara, Satoshi; Asamura, Kazushi +6 more

Electromagnetic plasma waves are thought to be responsible for energy exchange between charged particles in space plasmas. Such an energy exchange process is evidenced by phase space holes identified in the ion distribution function and measurements of the dot product of the plasma wave electric field and the ion velocity. We develop a method to i…

2017 Geophysical Research Letters
Cluster 21
Structured star formation in the Magellanic inter-Cloud region
DOI: 10.1093/mnras/stx2035 Bibcode: 2017MNRAS.472.2975M

Da Costa, G. S.; Belokurov, V.; Koposov, S. E. +5 more

We use a new contiguous imaging survey conducted using the Dark Energy Camera to investigate the distribution and properties of young stellar populations in the Magellanic inter-Cloud region. These young stars are strongly spatially clustered, forming a narrow chain of low-mass associations that trace the densest H I gas in the Magellanic Bridge a…

2017 Monthly Notices of the Royal Astronomical Society
Gaia 21
A low upper mass limit for the central black hole in the late-type galaxy NGC 4414
DOI: 10.1051/0004-6361/201629480 Bibcode: 2017A&A...597A..18T

Krajnović, D.; Emsellem, E.; McDermid, R. M. +7 more

We present our mass estimate of the central black hole in the isolated spiral galaxy NGC 4414. Using natural guide star adaptive optics assisted observations with the Gemini Near-Infrared Integral Field Spectrometer (NIFS) and the natural seeing Gemini Multi-Object Spectrographs-North (GMOS), we derived two-dimensional stellar kinematic maps of NG…

2017 Astronomy and Astrophysics
eHST 21
Evidence for Relativistic Disk Reflection in the Seyfert 1h Galaxy/ULIRG IRAS 05189-2524 Observed by NuSTAR and XMM-Newton
DOI: 10.3847/1538-4357/aa5df4 Bibcode: 2017ApJ...837...21X

Walton, Dominic J.; García, Javier A.; Harrison, Fiona A. +3 more

We present a spectral analysis of the NuSTAR and XMM-Newton observations of the Seyfert 1h galaxy/ULIRG IRAS 05189-2524 taken in 2013. We find evidence for relativistic disk reflection in the broadband X-ray spectrum: a highly asymmetric broad Fe Kα emission line extending down to 3 keV and a Compton scattering component above 10 keV. Physical mod…

2017 The Astrophysical Journal
XMM-Newton 21
Simultaneous Observations of p-mode Light Walls and Magnetic Reconnection Ejections above Sunspot Light Bridges
DOI: 10.3847/2041-8213/aa8edd Bibcode: 2017ApJ...848L...9H

Hou, Yijun; Li, Ting; Yang, Shuhong +2 more

Recent high-resolution observations from the Interface Region Imaging Spectrograph reveal bright wall-shaped structures in active regions (ARs), especially above sunspot light bridges. Their most prominent feature is the bright oscillating front in the 1400/1330 Å channel. These structures are named light walls and are often interpreted to be driv…

2017 The Astrophysical Journal
IRIS 21