Search Publications

Temporal Evolution of Solar Wind Ion Composition and their Source Coronal Holes during the Declining Phase of Cycle 23. I. Low-latitude Extension of Polar Coronal Holes
DOI: 10.1088/0004-637X/787/2/121 Bibcode: 2014ApJ...787..121K

Young, Peter R.; Wang, Yi-Ming; Ko, Yuan-Kuen +2 more

We analyzed 27 solar wind (SW) intervals during the declining phase of cycle 23, whose source coronal holes (CHs) can be unambiguously identified and are associated with one of the polar CHs. We found that the SW ions have a temporal trend of decreasing ionization state, and such a trend is different between the slow and fast SW. The photospheric …

2014 The Astrophysical Journal
SOHO 25
Constraining the Dust Coma Properties of Comet C/Siding Spring (2013 a1) at Large Heliocentric Distances
DOI: 10.1088/2041-8205/797/1/L8 Bibcode: 2014ApJ...797L...8L

Samarasinha, Nalin H.; A'Hearn, Michael F.; Li, Jian-Yang +5 more

The close encounter of comet C/2013 A1 (Siding Spring) with Mars on 2014 October 19 presented an extremely rare opportunity to obtain the first flyby quality data of the nucleus and inner coma of a dynamically new comet. However, the comet's dust tail potentially posed an impact hazard to those spacecraft orbiting Mars. To characterize the comet a…

2014 The Astrophysical Journal
eHST 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
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
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
Excitation of Kinetic Alfvén Waves by Fast Electron Beams
DOI: 10.1088/0004-637X/793/1/13 Bibcode: 2014ApJ...793...13C

Chen, L.; Wu, D. J.; Zhao, G. Q. +2 more

Energetic electron beams, which are ubiquitous in a large variety of active phenomena in space and astrophysical plasmas, are one of the most important sources that drive plasma instabilities. In this paper, taking account of the return-current effect of fast electron beams, kinetic Alfvén wave (KAW) instability driven by a fast electron beam is i…

2014 The Astrophysical Journal
Cluster 24
0.94-2.42 µm Ground-based Transmission Spectra of the Hot Jupiter HD-189733b
DOI: 10.1088/0004-637X/785/1/35 Bibcode: 2014ApJ...785...35D

Waldmann, I. P.; Tinetti, G.; Swain, M. R. +3 more

We present here new transmission spectra of the hot Jupiter HD-189733b using the SpeX instrument on the NASA Infrared Telescope Facility. We obtained two nights of observations where we recorded the primary transit of the planet in the J, H, and K bands simultaneously, covering a spectral range from 0.94 to 2.42 µm. We used Fourier analysis …

2014 The Astrophysical Journal
eHST 24
High Resolution X-Ray Spectroscopy of the Local Hot Gas along the 3C 273 Sightline
DOI: 10.1088/2041-8205/785/2/L24 Bibcode: 2014ApJ...785L..24F

Fang, Taotao; Jiang, Xiaochuan

X-ray observations of highly ionized metal absorption lines at z = 0 provide critical information on the hot gas distribution in and around the Milky Way. We present a study of more than 10 yr of Chandra and XMM-Newton observations of 3C 273, one of the brightest extragalactic X-ray sources. Compared with previous works, we obtain much tighter con…

2014 The Astrophysical Journal
XMM-Newton 24
Pre-flare Dynamics of Sunspot Groups
DOI: 10.1088/0004-637X/789/2/107 Bibcode: 2014ApJ...789..107K

Korsós, M. B.; Ludmány, A.; Baranyi, T.

Several papers provide evidence that the most probable sites of flare onset are the regions of high horizontal magnetic field gradients in solar active regions. Besides the localization of flare-producing areas, this work intends to reveal the characteristic temporal variations in these regions prior to flares. This study uses sunspot data instead…

2014 The Astrophysical Journal
SOHO 24
The Two-dimensional Spatial Distributions of the Globular Clusters and Low-mass X-Ray Binaries of NGC 4649
DOI: 10.1088/0004-637X/783/1/18 Bibcode: 2014ApJ...783...18D

Zezas, A.; Luo, B.; Fabbiano, G. +5 more

We report significant anisotropies in the projected two-dimensional (2D) spatial distributions of globular clusters (GCs) of the giant Virgo elliptical galaxy NGC 4649 (M60). Similar features are found in the 2D distribution of low-mass X-ray binaries (LMXBs), both associated with GCs and in the stellar field. Deviations from azimuthal symmetry su…

2014 The Astrophysical Journal
eHST 24