Search Publications

The Trace of the CNO Cycle in the Ring Nebula NGC 6888
DOI: 10.1088/0004-637X/785/2/100 Bibcode: 2014ApJ...785..100M

Morisset, C.; Bresolin, F.; García-Rojas, J. +3 more

We present new results on the chemical composition of the Galactic ring nebula NGC 6888 surrounding the WN6(h) star WR136. The data are based on deep spectroscopical observations taken with the High Dispersion Spectrograph at the 8.2 m Subaru Telescope. The spectra cover the optical range from 3700 to 7400 Å. The effect of the CNO cycle is well-id…

2014 The Astrophysical Journal
eHST 16
The Ultraviolet Attenuation Law in Backlit Spiral Galaxies
DOI: 10.1088/0004-6256/147/2/44 Bibcode: 2014AJ....147...44K

Holwerda, Benne W.; Schawinski, Kevin; Keel, William C. +2 more

The effective extinction law (attenuation behavior) in galaxies in the emitted ultraviolet (UV) regime is well known only for actively star-forming objects and combines effects of the grain properties, fine structure in the dust distribution, and relative distributions of stars and dust. We use Galaxy Evolution Explorer, XMM Optical Monitor, and H…

2014 The Astronomical Journal
XMM-Newton eHST 16
Insights into Titan's geology and hydrology based on enhanced image processing of Cassini RADAR data
DOI: 10.1002/2013JE004584 Bibcode: 2014JGRE..119.2149L

Lucas, Antoine; Aharonson, Oded; Hayes, Alexander G. +3 more

The Cassini Synthetic Aperture Radar has been acquiring images of Titan's surface since October 2004. To date, 59% of Titan's surface has been imaged by radar, with significant regions imaged more than once. Radar data suffer from speckle noise hindering interpretation of small-scale features and comparison of reimaged regions for change detection…

2014 Journal of Geophysical Research (Planets)
Cassini 16
The evolution of co-orbiting material in the orbit of 2201 Oljato from 1980 to 2012 as deduced from Pioneer Venus Orbiter and Venus Express magnetic records
DOI: 10.1111/maps.12102 Bibcode: 2014M&PS...49...28L

Zhang, Tielong; Russell, Christopher T.; Lai, Hairong +1 more

Asteroid 2201 Oljato passed through perihelion inside the orbit of Venus near the time of its conjunction with Venus in 1980, 1983, and 1986. During those three years, many interplanetary field enhancements (IFEs) were observed by the Pioneer Venus Orbiter (PVO) in the longitude sector where the orbit of Oljato lies inside Venus' orbit. We attribu…

2014 Meteoritics and Planetary Science
VenusExpress 16
A Gemini/GMOS study of the physical conditions and kinematics of the blue compact dwarf galaxy Mrk 996
DOI: 10.1051/0004-6361/201219270 Bibcode: 2014A&A...561A..64T

Thuan, Trinh X.; Izotov, Yuri I.; Carrasco, Eleazar R. +1 more


Aims: We present an integral field spectroscopic study with the Gemini Multi-Object Spectrograph (GMOS) of the unusual blue compact dwarf (BCD) galaxy Mrk 996.
Methods: We show through velocity and dispersion maps, emission-line intensity and ratio maps, and by a new technique of electron density limit imaging that the…

2014 Astronomy and Astrophysics
eHST 16
Spectral state transitions of the Ultraluminous X-ray Source IC 342 X-1
DOI: 10.1093/mnras/stu1471 Bibcode: 2014MNRAS.444..642M

Kaaret, P.; Mushotzky, R. F.; Miller, N. +6 more

We observed the Ultraluminous X-ray Source (ULX) IC 342 X-1 simultaneously in X-ray and radio with Chandra and the JVLA to investigate previously reported unresolved radio emission coincident with the ULX. The Chandra data reveal a spectrum that is much softer than observed previously and is well modelled by a thermal accretion disc spectrum. No s…

2014 Monthly Notices of the Royal Astronomical Society
XMM-Newton 16
XMM-Newton observation of the Galactic supernova remnant W51C (G49.1-0.1)
DOI: 10.1051/0004-6361/201323145 Bibcode: 2014A&A...563A...9S

Sasaki, Manami; Heinitz, Cornelia; Warth, Gabriele +1 more

Context. The supernova remnant (SNR) W51C is a Galactic object located in a strongly inhomogeneous interstellar medium with signs of an interaction of the SNR blast wave with dense molecular gas.
Aims: Diffuse X-ray emission from the interior of the SNR can reveal element abundances in the different emission regions and she…

2014 Astronomy and Astrophysics
XMM-Newton 16
The Ground-based H-, K-, and L-band Absolute Emission Spectra of HD 209458b
DOI: 10.1088/0004-637X/796/1/48 Bibcode: 2014ApJ...796...48Z

Zellem, Robert T.; Griffith, Caitlin A.; Swain, Mark R. +2 more

Here we explore the capabilities of NASA's 3.0 m Infrared Telescope Facility (IRTF) and SpeX spectrometer and the 5.08 m Hale telescope with the TripleSpec spectrometer with near-infrared H-, K-, and L-band measurements of HD 209458b's secondary eclipse. Our IRTF/SpeX data are the first absolute L-band spectroscopic emission measurements of any ex…

2014 The Astrophysical Journal
eHST 16
The role of ultraviolet imaging in studies of resolved and unresolved young stellar populations. M31 and M33
DOI: 10.1016/j.asr.2013.08.024 Bibcode: 2014AdSpR..53..928B

Bianchi, Luciana; Hodge, Paul; Williams, Benjamin +2 more

We discuss the relevance of UV data in the detection and characterization of hot massive stars and young stellar populations in galaxies. We show results from recent extensive surveys in M31 and M33 with Hubble Space Telescope (HST) multi-wavelength data including UV filters, which imaged several regions at a linear resolution (projected) of less …

2014 Advances in Space Research
eHST 16
IGR J17488-2338: a newly discovered giant radio galaxy
DOI: 10.1051/0004-6361/201423609 Bibcode: 2014A&A...565A...2M

Venturi, T.; Bird, A. J.; Ubertini, P. +4 more

We present the discovery of a large-scale radio structure associated with IGR J17488-2338, a source recently discovered by INTEGRAL and optically identified as a broad-line AGN at redshift 0.24. At low frequencies, the source properties are those of an intermediate-power FR II radio galaxy with a linear size of 1.4 Mpc. This new active galaxy is t…

2014 Astronomy and Astrophysics
INTEGRAL XMM-Newton 16