Search Publications

Multi-wavelength Emission from the Fermi Bubble. III. Stochastic (Fermi) Re-acceleration of Relativistic Electrons Emitted by SNRs
DOI: 10.1088/0004-637X/804/2/135 Bibcode: 2015ApJ...804..135C

Cheng, K. S.; Chernyshov, D. O.; Dogiel, V. A. +1 more

We analyze the model of stochastic re-acceleration of electrons that are emitted by supernova remnants (SNRs) in the Galactic Disk and then propagate into the Galactic Halo in order to explain the origin of nonthermal (radio and gamma-ray) emission from Fermi bubbles (FB). We assume that the energy for re-acceleration in the Halo is supplied by sh…

2015 The Astrophysical Journal
Planck 24
Resolved Millimeter Emission from the HD 15115 Debris Disk
DOI: 10.1088/0004-637X/801/1/59 Bibcode: 2015ApJ...801...59M

MacGregor, Meredith A.; Hughes, A. Meredith; Wilner, David J. +1 more

We have used the Submillimeter Array (SMA) to make 1.3 mm observations of the debris disk surrounding HD 15115, an F-type star with a putative membership in the β Pictoris moving group. This nearly edge-on debris disk shows an extreme asymmetry in optical scattered light, with an extent almost two times larger to the west of the star than to the e…

2015 The Astrophysical Journal
eHST 24
Exploring the Intrabinary Shock from the Redback Millisecond Pulsar PSR J2129-0429
DOI: 10.1088/2041-8205/801/2/L27 Bibcode: 2015ApJ...801L..27H

Cheng, K. S.; Takata, J.; Kong, A. K. H. +7 more

We have investigated the intrabinary shock emission from the redback millisecond pulsar PSR J2129-0429 with XMM-Newton and Fermi. Orbital modulation in X-ray and UV can be clearly seen. The X-ray modulation of this pulsar has a double-peaked structure with a dip in between. The observed X-rays are non-thermal dominant and can be modeled by a power…

2015 The Astrophysical Journal
XMM-Newton 24
Indications of R-mode Oscillations in SOHO/MDI Solar Radius Measurements
DOI: 10.1088/0004-637X/804/1/47 Bibcode: 2015ApJ...804...47S

Scargle, J. D.; Gough, D. O.; Sturrock, P. A. +1 more

Analysis of solar radius measurements acquired by the Michelson Doppler Imager on the Solar and Heliospheric Observatory spacecraft supports previously reported evidence of solar internal r-mode oscillations in Mt Wilson radius data and in 90Sr beta-decay data. The frequencies of these oscillations are compatible with oscillations in a …

2015 The Astrophysical Journal
SOHO 24
Physical Conditions of Coronal Plasma at the Transit of a Shock Driven by a Coronal Mass Ejection
DOI: 10.1088/0004-637X/812/2/119 Bibcode: 2015ApJ...812..119S

Bemporad, A.; Susino, R.; Mancuso, S.

We report here on the determination of plasma physical parameters across a shock driven by a coronal mass ejection using white light (WL) coronagraphic images and radio dynamic spectra (RDS). The event analyzed here is the spectacular eruption that occurred on 2011 June 7, a fast CME followed by the ejection of columns of chromospheric plasma, par…

2015 The Astrophysical Journal
SOHO 23
Short- and Long-Term Radio Variability of Young Stars in The Orion Nebula Cluster and Molecular Cloud
DOI: 10.1088/0004-637X/808/2/146 Bibcode: 2015ApJ...808..146R

Martín-Pintado, J.; Sanz-Forcada, J.; Chandler, C. J. +3 more

We have used the Karl G. Jansky Very Large Array (VLA) to carry out multi-epoch radio continuum monitoring of the Orion Nebula Cluster (ONC) and the background Orion Molecular Cloud (OMC; 3 epochs at Q band and 11 epochs at Ka band). Our new observations reveal the presence of 19 radio sources, mainly concentrated in the Trapezium Cluster and the …

2015 The Astrophysical Journal
eHST 23
N49: The First Robust Discovery of Recombining Plasma in an Extra-galactic Supernova Remnant
DOI: 10.1088/0004-637X/808/1/77 Bibcode: 2015ApJ...808...77U

Yamaguchi, Hiroya; Koyama, Katsuji; Uchida, Hiroyuki

Recent discoveries of recombining plasmas (RPs) in supernova remnants (SNRs) have dramatically changed our understanding of SNR evolution. To date, a dozen RP SNRs have been identified in the Galaxy. Here, we present Suzaku deep observations of four SNRs in the LMC, namely, N49, N49B, N23, and DEM L71, for accurate determination of their plasma st…

2015 The Astrophysical Journal
Suzaku 23
Herschel* Observations of Interstellar Chloronium. II. - Detections toward G29.96-0.02, W49N, W51, and W3(OH), and Determinations of the Ortho-to-Para and 35Cl/37Cl Isotopic Ratios
DOI: 10.1088/0004-637X/807/1/54 Bibcode: 2015ApJ...807...54N

Menten, Karl M.; Neufeld, David A.; Herbst, Eric +14 more

We report additional detections of the chloronium molecular ion, H2Cl+, toward four bright submillimeter continuum sources: G29.96-0.02, W49N, W51, and W3(OH). With the use of the HIFI instrument on board the Herschel Space Observatory, we observed the {2}12-{1}01 transition of ortho-H{}2

2015 The Astrophysical Journal
Herschel 23
The Three-mm Ultimate Mopra Milky Way Survey. II.Cloud and Star Formation near the Filamentary Ministarburst RCW 106
DOI: 10.1088/0004-637X/812/1/7 Bibcode: 2015ApJ...812....7N

Martin, Peter G.; Fuller, Gary A.; Barnes, Peter J. +10 more

We report here a study of gas, dust, and star formation rates (SFRs) in the molecular cloud complexes (MCCs) surrounding the giant H ii region RCW 106 using 12CO and 13CO(1-0) data from the Three-mm Ultimate Mopra Milky way Survey and archival data. We separate the emission in the Galactic Plane around l = 330°-335° and b = -…

2015 The Astrophysical Journal
Herschel 23
A Spectroscopic and Photometric Exploration of the C/M Ratio in the Disk of M31
DOI: 10.1088/0004-637X/810/1/60 Bibcode: 2015ApJ...810...60H

Williams, Benjamin F.; Gilbert, Karoline M.; Boyer, Martha L. +12 more

We explore the ratio (C/M) of carbon-rich to oxygen-rich thermally pulsing asymptotic giant branch (TP-AGB) stars in the disk of M31 using a combination of moderate-resolution optical spectroscopy from the Spectroscopic Landscape of Andromeda’s Stellar Halo survey and six-filter Hubble Space Telescope photometry from the Panchromatic Hubble Androm…

2015 The Astrophysical Journal
eHST 23