Search Publications

Proper Motions in Terzan 5: Membership of the Multi-iron Subpopulations and First Constraint on the Orbit
DOI: 10.1088/0004-637X/810/1/69 Bibcode: 2015ApJ...810...69M

Dalessandro, E.; Massari, D.; Rich, R. M. +6 more

By exploiting two sets of high-resolution images obtained with the Hubble Space Telescope Advanced Camera for Surveys/Wide Field Channel over a baseline of ∼10 years, we have measured relative proper motions (PMs) of ∼70,000 stars in the stellar system Terzan 5. The results confirm the membership of the three subpopulations with different iron abu…

2015 The Astrophysical Journal
eHST 30
A Two-ribbon White-light Flare Associated with a Failed Solar Eruption Observed by ONSET, SDO, and IRIS
DOI: 10.1088/0004-637X/809/1/46 Bibcode: 2015ApJ...809...46C

Cheng, X.; Ding, M. D.; Chen, P. F. +4 more

Two-ribbon brightenings are one of the most remarkable characteristics of an eruptive solar flare and are often used to predict the occurrence of coronal mass ejections (CMEs). Nevertheless, it was recently called into question whether all two-ribbon flares are eruptive. In this paper, we investigate a two-ribbon-like white-light (WL) flare that i…

2015 The Astrophysical Journal
IRIS 30
Formation and Eruption of a Small Flux Rope in the Chromosphere Observed by NST, IRIS, and SDO
DOI: 10.1088/0004-637X/809/1/83 Bibcode: 2015ApJ...809...83K

Wang, Haimin; Yurchyshyn, Vasyl; Kumar, Pankaj +1 more

Using high-resolution images from the 1.6 m New Solar Telescope at Big Bear Solar Observatory, we report the direct evidence of chromospheric reconnection at the polarity inversion line between two small opposite polarity sunspots. Small jetlike structures (with velocities of ∼20-55 km s-1) were observed at the reconnection site before …

2015 The Astrophysical Journal
IRIS 30
Binary Frequencies in a Sample of Globular Clusters. II. Sample Analysis and Comparison to Models
DOI: 10.1088/0004-637X/807/1/32 Bibcode: 2015ApJ...807...32J

Bregman, Joel N.; Ji, Jun

Binary stars are predicted to have an important role in the evolution of globular clusters, so we obtained binary fractions for 35 globular clusters that were imaged in the F606W and F814W with the Advanced Camera for Surveys on the Hubble Space Telescope. When compared to the values of prior efforts, we find significant discrepancies, despite eac…

2015 The Astrophysical Journal
eHST 30
Constraining the Redshift Evolution of the Cosmic Microwave Background Blackbody Temperature with PLANCK Data.
DOI: 10.1088/0004-637X/808/2/128 Bibcode: 2015ApJ...808..128D

Martins, C. J. A. P.; Kocevski, D.; Atrio-Barandela, F. +4 more

We constrain the deviation of adiabatic evolution of the universe using the data on the cosmic microwave background (CMB) temperature anisotropies measured by the Planck satellite and a sample of 481 X-ray selected clusters with spectroscopically measured redshifts. To avoid antenna beam effects, we bring all of the maps to the same resolution. We…

2015 The Astrophysical Journal
Planck 29
The Herschel Exploitation of Local Galaxy Andromeda (HELGA). VI. The Distribution and Properties of Molecular Cloud Associations in M31
DOI: 10.1088/0004-637X/798/1/58 Bibcode: 2015ApJ...798...58K

Fritz, J.; Cooray, A.; Lebouteiller, V. +18 more

In this paper we present a catalog of giant molecular clouds (GMCs) in the Andromeda (M31) galaxy extracted from the Herschel Exploitation of Local Galaxy Andromeda (HELGA) data set. GMCs are identified from the Herschel maps using a hierarchical source extraction algorithm. We present the results of this new catalog and characterize the spatial d…

2015 The Astrophysical Journal
Herschel 29
Estimating the Height of CMEs Associated with a Major SEP Event at the Onset of the Metric Type II Radio Burst during Solar Cycles 23 and 24
DOI: 10.1088/0004-637X/806/1/13 Bibcode: 2015ApJ...806...13M

Gopalswamy, N.; Yashiro, S.; Mäkelä, P. +2 more

We studied the coronal mass ejection (CME) height at the onset of 59 metric type II radio bursts associated with major solar energetic particle (SEP) events, excluding ground level enhancements (GLEs), during solar cycles 23 and 24. We calculated CME heights using a simple flare-onset method used by Gopalswamy et al. to estimate CME heights at the…

2015 The Astrophysical Journal
SOHO 29
Deceleration of Alpha Particles in the Solar Wind by Instabilities and the Rotational Force: Implications for Heating, Azimuthal Flow, and the Parker Spiral Magnetic Field
DOI: 10.1088/0004-637X/806/2/157 Bibcode: 2015ApJ...806..157V

Verscharen, Daniel; Hollweg, Joseph V.; Bourouaine, Sofiane +1 more

Protons and alpha particles in the fast solar wind are only weakly collisional and exhibit a number of non-equilibrium features, including relative drifts between particle species. Two non-collisional mechanisms have been proposed for limiting differential flow between alpha particles and protons: plasma instabilities and the rotational force. Bot…

2015 The Astrophysical Journal
Ulysses 29
Variable Reddening and Broad Absorption Lines in the Narrow-line Seyfert 1 Galaxy WPVS 007: An Origin in the Torus
DOI: 10.1088/2041-8205/809/1/L13 Bibcode: 2015ApJ...809L..13L

Komossa, S.; Terndrup, Donald M.; Leighly, Karen M. +2 more

We report the discovery of an occultation event in the low-luminosity narrow-line Seyfert 1 galaxy WPVS 007 in 2015 February and March. In concert with longer timescale variability, these observations place strong constraints on the nature and location of the absorbing material. Swift monitoring has revealed a secular decrease since ∼2010 accompan…

2015 The Astrophysical Journal
eHST 29
Correcting for Interplanetary Scattering in Velocity Dispersion analysis of Solar Energetic Particles
DOI: 10.1088/0004-637X/806/1/114 Bibcode: 2015ApJ...806..114L

Laitinen, T.; Valtonen, E.; Dalla, S. +1 more

To understand the origin of Solar Energetic Particles (SEPs), we must study their injection time relative to other solar eruption manifestations. Traditionally the injection time is determined using the Velocity Dispersion Analysis (VDA) where a linear fit of the observed event onset times at 1 AU to the inverse velocities of SEPs is used to deriv…

2015 The Astrophysical Journal
SOHO 29