Search Publications

Triggering Process of the X1.0 Three-ribbon Flare in the Great Active Region NOAA 12192
DOI: 10.3847/1538-4357/aa6682 Bibcode: 2017ApJ...838..134B

Kusano, Kanya; Shiota, Daikou; Inoue, Satoshi +1 more

The solar magnetic field in a flare-producing active region (AR) is much more complicated than theoretical models, which assume a very simple magnetic field structure. The X1.0 flare, which occurred in AR 12192 on 2014 October 25, showed a complicated three-ribbon structure. To clarify the trigger process of the flare and to evaluate the applicabi…

2017 The Astrophysical Journal
Hinode 27
ALMA Observations of the Interaction of a Radio Jet with Molecular Gas in Minkowski's Object
DOI: 10.3847/1538-4357/aa65d7 Bibcode: 2017ApJ...838..146L

Nyland, Kristina; Lacy, Mark; Croft, Steve +2 more

We use the Atacama Large Millimeter Array (ALMA) to detect and image CO (1-0) emission from Minkowski’s Object, a dwarf galaxy in the cluster Abell 194 that is interacting with a radio jet from a nearby elliptical galaxy. The ALMA observations, which are the first to detect molecular gas in Minkowski’s Object, also image the high-frequency continu…

2017 The Astrophysical Journal
eHST 27
A Potential Recoiling Supermassive Black Hole, CXO J101527.2+625911
DOI: 10.3847/1538-4357/aa6030 Bibcode: 2017ApJ...840...71K

Kim, D. -C.; Kim, Ji Hoon; Privon, G. C. +4 more

We have carried out a systematic search for recoiling supermassive black holes (rSMBH) using the Chandra Source and SDSS Cross-Match Catalog. From the survey, we have detected a potential rSMBH, CXO J101527.2+625911, at z = 0.3504. The source CXO J101527.2+625911 has a spatially offset (1.26 ± 0.05 kpc) active SMBH and kinematically offset broad e…

2017 The Astrophysical Journal
eHST 27
Characteristics that Produce White-light Enhancements in Solar Flares Observed by Hinode/SOT
DOI: 10.3847/1538-4357/aa9659 Bibcode: 2017ApJ...850..204W

Masuda, Satoshi; Watanabe, Kyoko; Kitagawa, Jun

To understand the conditions that produce white-light (WL) enhancements in solar flares, a statistical analysis of visible continuum data as observed by Hinode/Solar Optical Telescope (SOT) was performed. In this study, approximately 100 flare events from M- and X-class flares were selected. The time period during which the data were recorded span…

2017 The Astrophysical Journal
Hinode 27
Spectroscopy of Very Hot Plasma in Non-flaring Parts of a Solar Limb Active Region: Spatial and Temporal Properties
DOI: 10.3847/1538-4357/aa835f Bibcode: 2017ApJ...846...25P

Teriaca, Luca; Testa, Paola; Petralia, Antonino +4 more

In this work we investigate the thermal structure of an off-limb active region (AR) in various non-flaring areas, as it provides key information on the way these structures are heated. In particular, we concentrate on the very hot component (> 3 {MK}) as it is a crucial element to distinguish between different heating mechanisms. We present an …

2017 The Astrophysical Journal
Hinode SOHO 26
Heating of an Erupting Prominence Associated with a Solar Coronal Mass Ejection on 2012 January 27
DOI: 10.3847/1538-4357/aa79a4 Bibcode: 2017ApJ...844....3L

Moon, Yong-Jae; Reeves, Katharine K.; Raymond, John C. +2 more

We investigate the heating of an erupting prominence and loops associated with a coronal mass ejection and X-class flare. The prominence is seen as absorption in EUV at the beginning of its eruption. Later, the prominence changes to emission, which indicates heating of the erupting plasma. We find the densities of the erupting prominence using the…

2017 The Astrophysical Journal
Hinode SOHO 26
Stellar Stream Candidates in the Solar Neighborhood Found in the LAMOST DR3 and TGAS
DOI: 10.3847/1538-4357/aa7cf7 Bibcode: 2017ApJ...844..152L

Oswalt, T. D.; Zhao, G.; Zhang, L. +3 more

We have cross-matched the LAMOST DR3 with the Gaia DR1 TGAS catalogs and obtained a sample of 166,827 stars with reliable kinematics. A technique based on the wavelet transform was applied to detect significant overdensities in velocity space among five subsamples divided by spatial position. In total, 16 significant overdensities of stars with ve…

2017 The Astrophysical Journal
Gaia 26
Crowded Field Galaxy Photometry: Precision Colors in the CLASH Clusters
DOI: 10.3847/1538-4357/aa8ad5 Bibcode: 2017ApJ...848...37C

Koekemoer, Anton M.; Donahue, Megan; Voit, G. Mark +8 more

We present a new method for photometering objects in galaxy clusters. We introduce a mode-filtering technique for removing spatially variable backgrounds, improving both detection and photometric accuracy (roughly halving the scatter in the red sequence compared to previous catalogs of the same clusters). This method is based on robustly determini…

2017 The Astrophysical Journal
eHST 26
Chromospherically Active Stars in the RAVE Survey. II. Young Dwarfs in the Solar Neighborhood
DOI: 10.3847/1538-4357/835/1/61 Bibcode: 2017ApJ...835...61Z

Gilmore, G.; Freeman, K. C.; Munari, U. +19 more

A large sample of over 38,000 chromospherically active candidate solar-like stars and cooler dwarfs from the RAVE survey is addressed in this paper. An improved activity identification with respect to the previous study was introduced to build a catalog of field stars in the solar neighborhood with an excess emission flux in the calcium infrared t…

2017 The Astrophysical Journal
Gaia 26
Probing the Cold Dust Emission in the AB Aur Disk: A Dust Trap in a Decaying Vortex?
DOI: 10.3847/2041-8213/aa8558 Bibcode: 2017ApJ...846L...3F

Cernicharo, José; Fuente, Asunción; Baruteau, Clément +6 more

One serious challenge for planet formation is the rapid inward drift of pebble-sized dust particles in protoplanetary disks. Dust trapping at local maxima in the disk gas pressure has received much theoretical attention but still lacks observational support. The cold dust emission in the AB Aur disk forms an asymmetric ring at a radius of about 12…

2017 The Astrophysical Journal
Gaia 26