Search Publications

Evidence of scale height variations in the Martian ionosphere over the solar cycle
DOI: 10.1002/2015JA021949 Bibcode: 2015JGRA..12010913S

Lester, M.; Milan, S. E.; Morgan, D. D. +5 more

Solar cycle variations in solar radiation create density changes in any planetary ionosphere, which are well established in the Earth's case. At Mars, however, the ionospheric response to such changes is not well understood. We show the solar cycle impact on the topside ionosphere of Mars, using data from the Mars Advance Radar for Subsurface and …

2015 Journal of Geophysical Research (Space Physics)
MEx 24
Quiescent Compact Galaxies at Intermediate Redshift in the COSMOS Field. II. The Fundamental Plane of Massive Galaxies
DOI: 10.1088/0004-637X/806/1/122 Bibcode: 2015ApJ...806..122Z

Geller, Margaret J.; Damjanov, Ivana; Chilingarian, Igor +1 more

We examine the relation between surface brightness, velocity dispersion, and size—the fundamental plane (FP)—for quiescent galaxies at intermediate redshifts in the COSMOS field. The COSMOS sample consists of ∼150 massive quiescent galaxies with an average velocity dispersion of σ ∼ 250 km s-1 and redshifts between 0.2 < z < 0.8. …

2015 The Astrophysical Journal
eHST 24
An Observational Revisit of Band-split Solar Type-II Radio Bursts
DOI: 10.1088/0004-637X/812/1/52 Bibcode: 2015ApJ...812...52D

Li, Gang; Chen, Yao; Feng, Shiwei +3 more

The band split of solar type II radio bursts, discovered several decades ago, is a fascinating phenomenon, with the type II lanes exhibiting two almost parallel sub-bands with similar morphology. The underlying split mechanism remains elusive. One popular interpretation is that the splitting bands are emitted from the shock upstream and downstream…

2015 The Astrophysical Journal
SOHO 24
Identifying the source region of plasmaspheric hiss
DOI: 10.1002/2015GL063755 Bibcode: 2015GeoRL..42.3141L

Laakso, Harri; Masson, Arnaud; Escoubet, Philippe +4 more

The presence of the plasmaspheric hiss emission around the Earth has been known for more than 50 years, but its origin has remained unknown in terms of source location and mechanism. The hiss, made of whistler mode waves, exists for most of the time in the plasmasphere and is believed to control the radiation belt surrounding the Earth which makes…

2015 Geophysical Research Letters
Cluster 24
A CO-rich merger shaping a powerful and hyperluminous infrared radio galaxy at z = 2: the Dragonfly Galaxy
DOI: 10.1093/mnras/stv930 Bibcode: 2015MNRAS.451.1025E

Pentericci, L.; Colina, L.; Villar-Martín, M. +17 more

In the low-redshift Universe, the most powerful radio sources are often associated with gas-rich galaxy mergers or interactions. We here present evidence for an advanced, gas-rich (`wet') merger associated with a powerful radio galaxy at a redshift of z ∼ 2. This radio galaxy, MRC 0152-209, is the most infrared-luminous high-redshift radio galaxy …

2015 Monthly Notices of the Royal Astronomical Society
eHST 24
Modelling the atmosphere of the carbon-rich Mira RU Virginis
DOI: 10.1051/0004-6361/201526418 Bibcode: 2015A&A...583A.106R

Groenewegen, M. A. T.; Hron, J.; Paladini, C. +3 more

Context. We study the atmosphere of the carbon-rich Mira RU Vir using the mid-infrared high spatial resolution interferometric observations from VLTI/MIDI.
Aims: The aim of this work is to analyse the atmosphere of the carbon-rich Mira RU Vir with hydrostatic and dynamic models, in this way deepening the knowledge of the dy…

2015 Astronomy and Astrophysics
ISO 24
Circumstellar discs in Galactic centre clusters: Disc-bearing B-type stars in the Quintuplet and Arches clusters
DOI: 10.1051/0004-6361/201424132 Bibcode: 2015A&A...578A...4S

Ghez, A. M.; Anderson, J.; Brandner, W. +7 more

We investigate the circumstellar disc fraction as determined from L-band excess observations of the young, massive Arches and Quintuplet clusters residing in the central molecular zone of the Milky Way. The Quintuplet cluster was searched for L-band excess sources for the first time. We find a total of 26 excess sources in the Quintuplet cluster, …

2015 Astronomy and Astrophysics
eHST 24
Spectroscopic Observations of a Coronal Loop: Basic Physical Plasma Parameters Along the Full Loop Length
DOI: 10.1088/0004-637X/800/2/140 Bibcode: 2015ApJ...800..140G

Gupta, G. R.; Tripathi, Durgesh; Mason, Helen E.

Coronal loops are the basic structures of the solar transition region and corona. Understanding of the physical mechanisms behind the loop heating, plasma flows, and filling are still considered a major challenge in solar physics. The mechanism(s) should be able to supply mass to the corona from the chromosphere and to heat the plasma over 1 MK wi…

2015 The Astrophysical Journal
Hinode 24
Quadrupole-octopole alignment of CMB related to the primordial power spectrum with dipolar modulation in anisotropic spacetime
DOI: 10.1088/1674-1137/39/5/055101 Bibcode: 2015ChPhC..39e5101C

Wang, Sai; Chang, Zhe; Li, Xin

The WMAP and Planck observations show that the quadrupole and octopole orientations of the CMB might align with each other. We reveal that the quadrupole-octopole alignment is a natural implication of the primordial power spectrum in an anisotropic spacetime. The primordial power spectrum is presented with a dipolar modulation. We obtain the privi…

2015 Chinese Physics C
Planck 24
A Theoretical Study on the Vibrational Spectra of Polycyclic Aromatic Hydrocarbon Molecules with Aliphatic Sidegroups
DOI: 10.1088/0004-637X/801/1/34 Bibcode: 2015ApJ...801...34S

Zhang, Yong; Kwok, Sun; Sadjadi, SeyedAbdolreza

The role of aliphatic side groups in the formation of astronomical unidentified infrared emission (UIE) features is investigated by applying the density functional theory to a series of molecules with mixed aliphatic-aromatic structures. The effects of introducing various aliphatic groups to a fixed polycyclic aromatic hydrocarbon (PAH) core (oval…

2015 The Astrophysical Journal
ISO 24