Search Publications

Molecular Gas Kinematics and Star Formation Properties of the Strongly-lensed Quasar Host Galaxy RXS J1131-1231
DOI: 10.3847/1538-4357/aa5b98 Bibcode: 2017ApJ...836..180L

Riechers, Dominik A.; Pavesi, Riccardo; Leung, T. K. Daisy

We report observations of CO(J = 2 → 1) and {CO}(J=3\to 2) line emission toward the quadruply-lensed quasar RXS J1131-1231 at z = 0.654 obtained using the Plateau de Bure Interferometer (PdBI) and the Combined Array for Research in Millimeter-wave Astronomy (CARMA). Our lens modeling shows that the asymmetry in the double-horned CO(J = 2 → 1) line…

2017 The Astrophysical Journal
Herschel eHST 13
Spectroscopic study of the elusive globular cluster ESO452-SC11 and its surroundings
DOI: 10.1051/0004-6361/201730788 Bibcode: 2017A&A...604A..41K

Hansen, Camilla Juul; Kunder, Andrea; Koch, Andreas

Globular clusters (GCs) have long been recognized as being amongst the oldest objects in the Galaxy. As such, they have the potential of playing a pivotal role in deciphering the Milky Way's early history. Here we present the first spectroscopic study of the low-mass system ESO452-SC11 using the AAOmega multifibre spectrograph at medium resolution…

2017 Astronomy and Astrophysics
Gaia 13
The 1.1 mm Continuum Survey of the Small Magellanic Cloud: Physical Properties and Evolution of the Dust-selected Clouds
DOI: 10.3847/1538-4357/835/1/55 Bibcode: 2017ApJ...835...55T

Kohno, Kotaro; Yun, Min S.; Kawabe, Ryohei +18 more

The first 1.1 mm continuum survey toward the Small Magellanic Cloud (SMC) was performed using the AzTEC instrument installed on the ASTE 10 m telescope. This survey covered 4.5 deg2 of the SMC with 1σ noise levels of 5-12 mJy beam-1, and 44 extended objects were identified. The 1.1 mm extended emission has good spatial correl…

2017 The Astrophysical Journal
Herschel 13
The distance to the Galactic center determined by G, K, and M stars
DOI: 10.1007/s10509-017-3015-1 Bibcode: 2017Ap&SS.362...29B

Branham, Richard L.

The distance from the Sun to the center of the Galaxy R0 remains a fundamental parameter for Galactic structure. This study uses 105,275 G, K, and M stars of all luminosity classes with position, parallax, and proper motion taken …

2017 Astrophysics and Space Science
Hipparcos 13
Are Complex Magnetic Field Structures Responsible for the Confined X-class Flares in Super Active Region 12192?
DOI: 10.3847/1538-4357/aa7e7d Bibcode: 2017ApJ...845...54Z

Li, Ting; Zhang, Jun; Chen, Huadong

From 2014 October 19 to 27, six X-class flares occurred in super active region (AR) 12192. They were all confined flares and were not followed by coronal mass ejections. To examine the structures of the four flares close to the solar disk center from October 22 to 26, we firstly employ composite triple-time images in each flare process to display …

2017 The Astrophysical Journal
IRIS 13
Non-potential Field Formation in the X-shaped Quadrupole Magnetic Field Configuration
DOI: 10.3847/1538-4357/aa71a0 Bibcode: 2017ApJ...842..106K

Shimizu, T.; Inoue, S.; Kawabata, Y.

Some types of solar flares are observed in X-shaped quadrupolar field configuration. To understand the magnetic energy storage in such a region, we studied non-potential field formation in an X-shaped quadrupolar field region formed in the active region NOAA 11967, which produced three X-shaped M-class flares on 2014 February 2. Nonlinear force-fr…

2017 The Astrophysical Journal
Hinode 13
Long-term monitoring of comet 67P/Churyumov-Gerasimenko's jets with OSIRIS onboard Rosetta
DOI: 10.1093/mnras/stx1780 Bibcode: 2017MNRAS.469S.380S

Jorda, L.; Lamy, P. L.; Lara, L. M. +47 more

We used the OSIRIS camera system onboard the Rosetta spacecraft to monitor jet activity of comet 67P/Churyumov-Gerasimenko. With a monthly cadence, we covered an epoch from 2014 December to 2015 October, thereby including the first equinox and the perihelion passage. Jet features were measured in individual images, which were used to perform a sta…

2017 Monthly Notices of the Royal Astronomical Society
Rosetta 13
Beyond 3 au from the Sun: The Hypervolatiles CH4, C2H6, and CO in the Distant Comet C/2006 W3 (Christensen)
DOI: 10.3847/1538-3881/aa64dd Bibcode: 2017AJ....153..241B

Villanueva, Geronimo L.; Mumma, Michael J.; DiSanti, Michael A. +5 more

Comet C/2006 W3 (Christensen) remained outside a heliocentric distance (R h) of 3.1 au throughout its apparition, but it presented an exceptional opportunity to directly sense a suite of molecules released from its nucleus. The Cryogenic Infrared Echelle Spectrograph at ESO-VLT detected infrared emissions from the three “hypervolatiles”…

2017 The Astronomical Journal
Herschel Rosetta 13
A Large Catalog of Homogeneous Ultra-Violet/Optical GRB Afterglows: Temporal and Spectral Evolution
DOI: 10.3847/1538-4365/228/2/13 Bibcode: 2017ApJS..228...13R

Gronwall, Caryl; Kuin, N. P. M.; Roming, Peter W. A. +10 more

We present the second Swift Ultra-Violet/Optical Telescope (UVOT) gamma-ray burst (GRB) afterglow catalog, greatly expanding on the first Swift UVOT GRB afterglow catalog. The second catalog is constructed from a database containing over 120,000 independent UVOT observations of 538 GRBs first detected by Swift, the High Energy Transient Explorer 2…

2017 The Astrophysical Journal Supplement Series
INTEGRAL 13
On the east-west longitudinally asymmetric distribution of solar proton events
DOI: 10.1093/mnras/stw2255 Bibcode: 2017MNRAS.464...85H

Wan, W.; He, H. -Q.

A large data set of 78 solar proton events observed near the Earth's orbit during 1996-2011 is investigated. An east-west longitudinal (azimuthal) asymmetry is found to exist in the distribution of flare sources of solar proton events. With the same longitudinal separation between the flare sources and the magnetic field line footpoint of observer…

2017 Monthly Notices of the Royal Astronomical Society
SOHO 13