Search Publications

J- and H-band Imaging of AKARI North Ecliptic Pole Survey Field
DOI: 10.1088/0067-0049/214/2/20 Bibcode: 2014ApJS..214...20J

Im, Myungshin; Matsuhara, Hideo; Lee, Hyung Mok +2 more

We present the J- and H-band source catalog covering the AKARI North Ecliptic Pole field. Filling the gap between the optical data from other follow-up observations and mid-infrared (MIR) data from AKARI, our near-infrared (NIR) data provides contiguous wavelength coverage from optical to MIR. For the J- and H-band imaging, we used the FLoridA Mul…

2014 The Astrophysical Journal Supplement Series
AKARI 25
How Can Active Region Plasma Escape into the Solar Wind from Below a Closed Helmet Streamer?
DOI: 10.1007/s11207-014-0582-y Bibcode: 2014SoPh..289.4151M

Pick, M.; Mandrini, C. H.; van Driel-Gesztelyi, L. +6 more

Recent studies show that active-region (AR) upflowing plasma, observed by the EUV-Imaging Spectrometer (EIS) onboard Hinode, can gain access to open-field lines and be released into the solar wind (SW) via magnetic-interchange reconnection at magnetic null-points in pseudo-streamer configurations. When only one bipolar AR is present on the Sun and…

2014 Solar Physics
Hinode SOHO 25
Non-steady state tidal heating of Enceladus
DOI: 10.1016/j.icarus.2014.03.006 Bibcode: 2014Icar..235...75S

Kurita, K.; Hussmann, H.; Shoji, D. +1 more

Enceladus is one of the most geologically active bodies in the Solar System. The satellite's diverse surface suggests that Enceladus was subject to past episodic heating. It is largely probable that the activity of Enceladus is not in a steady state. In order to analyze the non-steady state heating, thermal and orbital coupled calculation is neede…

2014 Icarus
Cassini 25
Polycyclic aromatic hydrocarbon feature deficit of starburst galaxies in the AKARI North Ecliptic Pole Deep field
DOI: 10.1051/0004-6361/201423744 Bibcode: 2014A&A...566A.136M

Inami, H.; Armus, L.; Serjeant, S. +6 more

We study the behaviour of polycyclic aromatic hydrocarbon (PAH) emission in galaxies at z = 0.3-1.4 using 1868 samples from the revised catalogue of AKARI North Ecliptic Pole Deep survey. The continuous filter coverage at 2-24 µm makes it possible to measure 8 µm luminosity, which is dominated by PAH emission, for galaxies at up to z =…

2014 Astronomy and Astrophysics
AKARI 25
Hubble Space Telescope Observations and Geometric Models of Compact Multipolar Planetary Nebulae
DOI: 10.1088/0004-637X/787/1/25 Bibcode: 2014ApJ...787...25H

Zhang, Yong; Kwok, Sun; Hsia, Chih-Hao +1 more

We report high angular resolution Hubble Space Telescope observations of 10 compact planetary nebulae (PNs). Many interesting internal structures, including multipolar lobes, arcs, two-dimensional rings, tori, and halos, are revealed for the first time. These results suggest that multipolar structures are common among PNs, and these structures dev…

2014 The Astrophysical Journal
IUE eHST 25
Pair separation of magnetic elements in the quiet Sun
DOI: 10.1051/0004-6361/201424380 Bibcode: 2014A&A...569A.121G

Gošić, M.; Orozco Suárez, D.; Bellot Rubio, L. +5 more

The dynamic properties of the quiet Sun photosphere can be investigated by analyzing the pair dispersion of small-scale magnetic fields (i.e., magnetic elements). By using 25 h-long Hinode magnetograms at high spatial resolution (0.3 arcsec), we tracked 68 490 magnetic element pairs within a supergranular cell near the disk center. The computed pa…

2014 Astronomy and Astrophysics
Hinode 24
Helioseismology of Pre-emerging Active Regions. III. Statistical Analysis
DOI: 10.1088/0004-637X/786/1/19 Bibcode: 2014ApJ...786...19B

Leka, K. D.; Barnes, G.; Birch, A. C. +1 more

The subsurface properties of active regions (ARs) prior to their appearance at the solar surface may shed light on the process of AR formation. Helioseismic holography has been applied to samples taken from two populations of regions on the Sun (pre-emergence and without emergence), each sample having over 100 members, that were selected to minimi…

2014 The Astrophysical Journal
SOHO 24
The Sun's Interior Structure and Dynamics, and the Solar Cycle
DOI: 10.1007/s11214-014-0101-3 Bibcode: 2014SSRv..186..191B

Thompson, M. J.; Howe, R.; Broomhall, A. -M. +2 more

The Sun's internal structure and dynamics can be studied with helioseismology, which uses the Sun's natural acoustic oscillations to build up a profile of the solar interior. We discuss how solar acoustic oscillations are affected by the Sun's magnetic field. Careful observations of these effects can be inverted to determine the variations in the …

2014 Space Science Reviews
SOHO 24
Inflationary generalized Chaplygin gas and dark energy in light of the Planck and BICEP2 experiments
DOI: 10.1103/PhysRevD.90.083515 Bibcode: 2014PhRvD..90h3515D

Kumar, Sumit; Dinda, Bikash R.; Sen, Anjan A.

In this work, we study an inflationary scenario in the presence of generalized Chaplygin gas (GCG). We show that in Einstein gravity, GCG is not a suitable candidate for inflation; but in a five-dimensional brane-world scenario, it can work as a viable inflationary model. We calculate the relevant quantities such as ns, r, and As

2014 Physical Review D
Planck 24
On the Nature of the Deeply Embedded Protostar OMC-2 FIR 4
DOI: 10.1088/0004-637X/786/1/26 Bibcode: 2014ApJ...786...26F

Manoj, P.; Megeath, S. T.; Osorio, M. +7 more

We use mid-infrared to submillimeter data from the Spitzer, Herschel, and Atacama Pathfinder Experiment telescopes to study the bright submillimeter source OMC-2 FIR 4. We find a point source at 8, 24, and 70 µm, and a compact, but extended source at 160, 350, and 870 µm. The peak of the emission from 8 to 70 µm, attributed to th…

2014 The Astrophysical Journal
Herschel 24