Search Publications

Eskers in a complete, wet-based glacial system in the Phlegra Montes region, Mars
DOI: 10.1016/j.epsl.2015.09.023 Bibcode: 2015E&PSL.431...96G

Balme, Matthew; Gallagher, Colman

Although glacial landsystems produced under warm/wet based conditions are very common on Earth, even here, observations of subglacial landforms such as eskers emerging from extant glaciers are rare. This paper describes a system of sinuous ridges emerging from the in situ but now degraded piedmont terminus of a Late Amazonian-aged (∼150 Ma) glacie…

2015 Earth and Planetary Science Letters
MEx 33
Using FUV to IR Variability to Probe the Star-Disk Connection in the Transitional Disk of GM Aur
DOI: 10.1088/0004-637X/805/2/149 Bibcode: 2015ApJ...805..149I

Sitko, Michael; Calvet, Nuria; Ingleby, Laura +3 more

We analyze three epochs of ultraviolet, optical, and near-infrared (NIR) observations of the Taurus transitional disk GM Aur using the Hubble Space Telescope Imaging Spectrograph (STIS) and the Infrared Telescope Facility SpeX spectrograph. Observations were separated by one week and three months in order to study variability over multiple timesca…

2015 The Astrophysical Journal
eHST 33
Brightest cluster galaxies in the extended GMRT radio halo cluster sample. Radio properties and cluster dynamics
DOI: 10.1051/0004-6361/201526341 Bibcode: 2015A&A...581A..23K

Kale, R.; Giacintucci, S.; Venturi, T. +4 more


Aims: First-ranked galaxies in clusters, usually referred to as brightest cluster galaxies (BCGs), show exceptional properties over the whole electromagnetic spectrum. They are the most massive elliptical galaxies and show the highest probability to be radio loud. Moreover, their special location at the centres of galaxy clusters raises the q…

2015 Astronomy and Astrophysics
XMM-Newton 33
Dust-to-gas ratio, XCO factor and CO-dark gas in the Galactic anticentre: an observational study
DOI: 10.1093/mnras/stv103 Bibcode: 2015MNRAS.448.2187C

Huang, Y.; Chen, B. -Q.; Xiang, M. -S. +2 more

We investigate the correlation between extinction and H I and CO emission at intermediate and high Galactic latitudes (|b| > 10°) within the footprint of the Xuyi Schmidt Telescope Photometric Survey of the Galactic anticentre (XSTPS-GAC) on small and large scales. In Paper I, we present a three-dimensional (3D) dust extinction map within the f…

2015 Monthly Notices of the Royal Astronomical Society
Planck 33
Reapproaching the Spin Estimate of GX 339-4
DOI: 10.1088/0004-637X/806/2/262 Bibcode: 2015ApJ...806..262L

Miller, J. M.; Cackett, E. M.; Ludlam, R. M.

We systematically reanalyze two previous observations of the black hole (BH) GX 339-4 in the very high and intermediate state taken with XMM-Newton and Suzaku. We utilize up-to-date data reduction procedures and implement the recently developed, self-consistent model for X-ray reflection and relativistic ray tracing, relxill. In the very high and …

2015 The Astrophysical Journal
Suzaku XMM-Newton 33
Vertical propagation of planetary-scale waves in variable background winds in the upper cloud region of Venus
DOI: 10.1016/j.icarus.2014.07.011 Bibcode: 2015Icar..248..560K

Futaana, Yoshifumi; Imamura, Takeshi; Kouyama, Toru +2 more

Recently it was found that the low-latitude zonal wind and the amplitudes of Kelvin and Rossby waves at the cloud top of Venus show long-term variations in a synchronized manner. For the purpose of explaining this synchronization, we investigated the influence of the background zonal wind profile on the upward propagation of Kelvin and Rossby wave…

2015 Icarus
VenusExpress 33
The analysis of realistic stellar Gaia mock catalogues - I. Red clump stars as tracers of the central bar
DOI: 10.1093/mnras/stu2457 Bibcode: 2015MNRAS.447..218R

Figueras, F.; Antoja, T.; Romero-Gómez, M. +2 more

In this first paper, we simulate the population of disc red clump stars to be observed by Gaia. We generate a set of test particles and we evolve it in a 3D barred Milky Way like galactic potential. We assign physical properties of the red clump trace population and a realistic 3D interstellar extinction model. We add Gaia observational constraint…

2015 Monthly Notices of the Royal Astronomical Society
Gaia 33
Interannual and seasonal changes in the north polar ice deposits of Mars: Observations from MY 29-31 using MARCI
DOI: 10.1016/j.icarus.2014.08.026 Bibcode: 2015Icar..251..181C

James, P. B.; Cantor, B. A.; Calvin, W. M. +1 more

The MARCI camera on the Mars Reconnaissance Orbiter provides daily synoptic coverage that allows monitoring of seasonal cap retreat and interannual changes that occur between Mars year (MY) and over the northern summer. The northern seasonal cap evolution was observed in MY 29, 30 and 31 (12/2007-04/2012). Observation over multiple Mars years allo…

2015 Icarus
eHST 33
Short-period X-ray oscillations in super-soft novae and persistent super-soft sources
DOI: 10.1051/0004-6361/201425178 Bibcode: 2015A&A...578A..39N

Ness, J. -U.; Henze, M.; Wilms, J. +10 more

Context. Transient short-period (<100 s) oscillations have been found in the X-ray light curves of three novae during their super-soft source (SSS) phase and in one persistent SSS.
Aims: We pursue an observational approach to determine possible driving mechanisms and relations to fundamental system parameters such as the white dwarf mass. …

2015 Astronomy and Astrophysics
XMM-Newton 33
The Tip of the Red Giant Branch Distances to Type Ia Supernova Host Galaxies. III. NGC 4038/39 and NGC 5584
DOI: 10.1088/0004-637X/807/2/133 Bibcode: 2015ApJ...807..133J

Lee, Myung Gyoon; Jang, In Sung

We present the tip of the red giant branch (TRGB) distances to Type Ia supernova (SNe Ia) host galaxies NGC 4038/39 and NGC 5584. Based on the deep images constructed using archival Hubble Space Telescope data, we detect red giant branch stars in each galaxy. VI photometry of the resolved stars and corresponding I-band luminosity functions show th…

2015 The Astrophysical Journal
eHST 33