Search Publications

The Blue Straggler Star Population in NGC 1261: Evidence for a Post-core-collapse Bounce State
DOI: 10.1088/2041-8205/795/1/L10 Bibcode: 2014ApJ...795L..10S

Sills, Alison; Puzia, Thomas H.; Simunovic, Mirko

We present a multi-passband photometric study of the Blue Straggler Star (BSS) population in the Galactic globular cluster (GC) NGC 1261, using available space- and ground-based survey data. The inner BSS population is found to have two distinct sequences in the color-magnitude diagram (CMD), similar to double BSS sequences detected in other GCs. …

2014 The Astrophysical Journal
eHST 36
Cross-calibration of the XMM-Newton EPIC pn and MOS on-axis effective areas using 2XMM sources
DOI: 10.1051/0004-6361/201423422 Bibcode: 2014A&A...564A..75R

Read, A. M.; Guainazzi, M.; Sembay, S.


Aims: We aim to examine the relative cross-calibration accuracy of the on-axis effective areas of the XMM-Newton EPIC pn and MOS instruments.
Methods: Spectra from a sample of 46 bright, high-count, non-piled-up, isolated on-axis point sources are stacked together, and model residuals are examined to characterize the EPIC MOS-to-pn inter…

2014 Astronomy and Astrophysics
XMM-Newton 36
The debris disc of solar analogue τ Ceti: Herschel observations and dynamical simulations of the proposed multiplanet system
DOI: 10.1093/mnras/stu1641 Bibcode: 2014MNRAS.444.2665L

Heras, A. M.; Fridlund, M.; Blommaert, J. A. D. L. +16 more

τ Ceti is a nearby, mature G-type star very similar to our Sun, with a massive Kuiper Belt analogue and possible multiplanet system that has been compared to our Solar system. We present Herschel Space Observatory images of the debris disc, finding the disc is resolved at 70 µm and 160 µm, and marginally resolved at 250 µm. The H…

2014 Monthly Notices of the Royal Astronomical Society
AKARI Herschel 36
Herschel HIFI Observations of O2 toward Orion: Special Conditions for Shock Enhanced Emission
DOI: 10.1088/0004-637X/793/2/111 Bibcode: 2014ApJ...793..111C

Caselli, Paola; Viti, Serena; Encrenaz, Pierre +18 more

We report observations of molecular oxygen (O2) rotational transitions at 487 GHz, 774 GHz, and 1121 GHz toward Orion Peak A. The O2 lines at 487 GHz and 774 GHz are detected at velocities of 10-12 km s-1 with line widths ~3 km s-1 however, the transition at 1121 GHz is not detected. The observed line ch…

2014 The Astrophysical Journal
Herschel 36
Jupiter's equatorward auroral features: Possible signatures of magnetospheric injections
DOI: 10.1002/2014JA020527 Bibcode: 2014JGRA..11910068D

Bonfond, B.; Gérard, J. -C.; Grodent, D. +2 more

The present study investigates the characteristics of ultraviolet auroral features located equatorward of the main emission appearing in Hubble Space Telescope images of the northern and southern Jovian hemispheres obtained in 2000-2007. On average, one feature is observed every day, but several auroral structures are occasionally seen over a wide…

2014 Journal of Geophysical Research (Space Physics)
eHST 36
Ultraluminous Infrared Galaxies in the AKARI All-sky Survey
DOI: 10.1088/0004-637X/797/1/54 Bibcode: 2014ApJ...797...54K

Goto, T.; Doi, Y.; Kilerci Eser, E.

We present a new catalog of 118 ultraluminous infrared galaxies (ULIRGs) and one hyperluminous infrared galaxy (HLIRG) by cross-matching the AKARI all-sky survey with the Sloan Digital Sky Survey Data Release 10 (SDSS DR10) and the final data release of the Two-Degree Field Galaxy Redshift Survey. Forty of the ULIRGs and one HLIRG are new identifi…

2014 The Astrophysical Journal
AKARI 36
Physical and dynamical properties of the main belt triple Asteroid (87) Sylvia
DOI: 10.1016/j.icarus.2014.05.046 Bibcode: 2014Icar..239..118B

Berthier, J.; Carry, B.; Marchis, F. +2 more

We present the analysis of high angular resolution observations of the triple Asteroid (87) Sylvia collected with three 8-10 m class telescopes (Keck, VLT, Gemini North) and the Hubble Space Telescope. The moons’ mutual orbits were derived individually using a purely Keplerian model. We computed the position of Romulus, the outer moon of the syste…

2014 Icarus
eHST 36
Revealing the Location and Structure of the Accretion Disk Wind in PDS 456
DOI: 10.1088/0004-637X/784/1/77 Bibcode: 2014ApJ...784...77G

Turner, T. J.; Reeves, J. N.; Braito, V. +7 more

We present evidence for the rapid variability of the high-velocity iron K-shell absorption in the nearby (z = 0.184) quasar PDS 456. From a recent long Suzaku observation in 2013 (~1 Ms effective duration), we find that the equivalent width of iron K absorption increases by a factor of ~5 during the observation, increasing from <105 eV within t…

2014 The Astrophysical Journal
Suzaku 36
Spectral and temporal properties of RX J0520.5-6932 (LXP 8.04) during a type-I outburst
DOI: 10.1051/0004-6361/201423934 Bibcode: 2014A&A...567A.129V

Haberl, F.; Udalski, A.; Sturm, R. +2 more


Aims: We observed RX J0520.5-6932 in the X-rays and studied the optical light curve of its counterpart to verify it as a Be/X-ray binary.
Methods: We performed an XMM-Newton anticipated target-of-opportunity observation in January 2013 during an X-ray outburst of the source in order to search for pulsations and derive its spectral proper…

2014 Astronomy and Astrophysics
XMM-Newton 36
Lupus I Observations from the 2010 Flight of the Balloon-borne Large Aperture Submillimeter Telescope for Polarimetry
DOI: 10.1088/0004-637X/784/2/116 Bibcode: 2014ApJ...784..116M

Ward-Thompson, Derek; Fissel, Laura M.; Savini, Giorgio +29 more

The Balloon-borne Large Aperture Submillimeter Telescope for Polarimetry (BLASTPol) was created by adding polarimetric capability to the BLAST experiment that was flown in 2003, 2005, and 2006. BLASTPol inherited BLAST's 1.8 m primary and its Herschel/SPIRE heritage focal plane that allows simultaneous observation at 250, 350, and 500 µm. We…

2014 The Astrophysical Journal
Herschel 36