Search Publications

Detecting gravitationally lensed Population III galaxies with the Hubble Space Telescope and the James Webb Space Telescope
DOI: 10.1111/j.1365-2966.2012.22078.x Bibcode: 2012MNRAS.427.2212Z

Broadhurst, Tom; Schaerer, Daniel; Östlin, Göran +6 more

Small galaxies consisting entirely of Population III (pop III) stars may form at high redshifts, and could constitute one of the best probes of such stars. Here, we explore the prospects of detecting gravitationally lensed pop III galaxies behind the galaxy cluster J0717.5+3745 (J0717) with both the Hubble Space Telescope (HST) and the upcoming Ja…

2012 Monthly Notices of the Royal Astronomical Society
eHST 52
Suzaku Observations of the Hydra A Cluster out to the Virial Radius
DOI: 10.1093/pasj/64.5.95 Bibcode: 2012PASJ...64...95S

Sato, Kosuke; Fukazawa, Yasushi; Nakazawa, Kazuhiro +12 more

We report on Suzaku observations of the northern half of the Hydra A cluster out to ∼ 1.4 Mpc, reaching the virial radius. There are the first Suzaku observations of a medium-size (kT ∼ 3 keV) cluster out to the virial radius. Two observations were conducted, north-west and north-east offsets, which continue in a filament direction and a void dire…

2012 Publications of the Astronomical Society of Japan
Suzaku XMM-Newton 52
A 30 AU Radius CO Gas Hole in the Disk around the Herbig Ae Star Oph IRS 48
DOI: 10.1088/0004-637X/744/2/116 Bibcode: 2012ApJ...744..116B

van Dishoeck, E. F.; Pontoppidan, K. M.; Herczeg, G. J. +1 more

The physical processes leading to the disappearance of disks around young stars are not well understood. A subclass of transitional disks, the so-called cold disks with large inner dust holes, provides a crucial laboratory for studying disk dissipation processes. IRS 48 has a 30 AU radius hole previously measured from dust continuum imaging at 18.…

2012 The Astrophysical Journal
eHST 52
On the metallicity dependence of crystalline silicates in oxygen-rich asymptotic giant branch stars and red supergiants
DOI: 10.1111/j.1365-2966.2012.21978.x Bibcode: 2012MNRAS.427.3209J

Zijlstra, A. A.; Boyer, M. L.; Gielen, C. +10 more

We investigate the occurrence of crystalline silicates in oxygen-rich evolved stars across a range of metallicities and mass-loss rates. It has been suggested that the crystalline silicate feature strength increases with increasing mass-loss rate, implying a correlation between lattice structure and wind density. To test this, we analyse Spitzer I…

2012 Monthly Notices of the Royal Astronomical Society
ISO 52
Interpretation of combined infrared, submillimeter, and millimeter thermal flux data obtained during the Rosetta fly-by of Asteroid (21) Lutetia
DOI: 10.1016/j.icarus.2012.08.002 Bibcode: 2012Icar..221..395K

Capaccioni, F.; Lee, S.; Hofstadter, M. +9 more

The European Space Agency’s Rosetta spacecraft is the first Solar System mission to include instrumentation capable of measuring planetary thermal fluxes at both near-IR (VIRTIS) and submillimeter-millimeter (smm-mm, MIRO) wavelengths. Its primary mission is a 1 year reconnaissance of Comet 67P/Churyumov-Gerasimenko beginning in 2014. During a 201…

2012 Icarus
Rosetta 52
The Coronal Source of Extreme-ultraviolet Line Profile Asymmetries in Solar Active Region Outflows
DOI: 10.1088/2041-8205/760/1/L5 Bibcode: 2012ApJ...760L...5B

Warren, Harry P.; Brooks, David H.

High-resolution spectra from the Hinode EUV Imaging Spectrometer have revealed that coronal spectral line profiles are sometimes asymmetric, with a faint enhancement in the blue wing on the order of 100 km s-1. These asymmetries could be important since they may be subtle yet diagnostically useful signatures of coronal heating or solar …

2012 The Astrophysical Journal
Hinode 52
A broad iron line in LMC X-1
DOI: 10.1111/j.1365-2966.2012.22128.x Bibcode: 2012MNRAS.427.2552S

Steiner, James F.; Reis, Rubens C.; Fabian, Andrew C. +6 more

We present results from a deep Suzaku observation of the black hole in LMC X-1, supplemented by coincident monitoring with the Rossi X-ray Timing Explorer (RXTE). We identify broad relativistic reflection features in a soft disc-dominated spectrum. A strong and variable power-law component of emission is present which we use to demonstrate that en…

2012 Monthly Notices of the Royal Astronomical Society
Suzaku 52
An extension of the DUSTY radiative transfer code and an application to OH 26.5 and TT Cygni
DOI: 10.1051/0004-6361/201218965 Bibcode: 2012A&A...543A..36G

Groenewegen, M. A. T.

For the best-studied nearby Galactic asymptotic giant branch (AGB) stars a wealth of observational data is typically available in the form of photometry, often extending into the sub-mm, spectra covering a wide wavelength range, and often also visibility curves. Almost 100 AGB stars and red super giants have been imaged as part of the MESS Hersche…

2012 Astronomy and Astrophysics
ISO 52
The nucleus of Comet 67P/Churyumov-Gerasimenko. A new shape model and thermophysical analysis
DOI: 10.1051/0004-6361/201220116 Bibcode: 2012A&A...548A..12L

Lowry, S.; Snodgrass, C.; Green, S. F. +5 more

Context. Comet 67P/Churyumov-Gerasimenko is the target of the European Space Agency Rosetta spacecraft rendez-vous mission. Detailed physical characteristation of the comet before arrival is important for mission planning as well as providing a test bed for ground-based observing and data-analysis methods.
Aims: To conduct a long-term observa…

2012 Astronomy and Astrophysics
Rosetta eHST 52
Vertical structure of the Venus cloud top from the VeRa and VIRTIS observations onboard Venus Express
DOI: 10.1016/j.icarus.2011.07.001 Bibcode: 2012Icar..217..599L

Pätzold, M.; Drossart, P.; Piccioni, G. +6 more

We investigate the Venus cloud top structure by joint analysis of the data from Visual and Thermal Infrared Imaging Spectrometer (VIRTIS) and the atmospheric temperature sounding by the Radio Science experiment (VeRa) onboard Venus Express. The cloud top altitude and aerosol scale height are derived by fitting VIRTIS spectra at 4-5 µm with t…

2012 Icarus
VenusExpress 52