Search Publications

Modeling the distribution of H2O and HDO in the upper atmosphere of Venus
DOI: 10.1029/2008JE003095 Bibcode: 2009JGRE..114.0B28L

Liang, Mao-Chang; Yung, Yuk L.

The chemical and dynamical processes in the upper atmosphere of Venus are poorly known. Recently obtained vertical profiles of trace species from the Venus Express mission, such as HCl, H2O, and HDO, provide new information to constrain these processes. Here, we simulate these profiles, using the model we have developed and described in…

2009 Journal of Geophysical Research (Planets)
VenusExpress 16
Discovery of a large and bright bow shock nebula associated with low-mass X-ray binary SAX J1712.6-3739
DOI: 10.1111/j.1745-3933.2009.00643.x Bibcode: 2009MNRAS.397L...6W

Read, A. M.; Degenaar, N.; Wijnands, R. +6 more

In a multiwavelength programme dedicated to identifying optical counterparts of faint persistent X-ray sources in the Galactic bulge, we find an accurate X-ray position of SAX J1712.6-3739 through Chandra observations, and discover its faint optical counterpart using our data from EFOSC2 on the ESO 3.6-m telescope. We find this source to be a high…

2009 Monthly Notices of the Royal Astronomical Society
XMM-Newton 16
Suzaku and XMM-Newton Observations of Diffuse X-Ray Emission from the Eastern Tip Region of the Carina Nebula
DOI: 10.1093/pasj/61.sp1.S123 Bibcode: 2009PASJ...61S.123E

Hamaguchi, Kenji; Corcoran, Michael F.; Petre, Robert +3 more

The eastern tip region of the Carina Nebula was observed with the Suzaku XIS for 77ks to conduct a high-precision spectral study of extended X-ray emission. XMM-Newton EPIC data of this region were also utilized to detect point sources. The XIS detected strong extended X-ray emission from the entire field-of-view with a 0.2--5keV flux of 0.7--4 × …

2009 Publications of the Astronomical Society of Japan
Suzaku XMM-Newton 16
Spatial Distributions of Absorption, Local Suppression, and Emissivity Reduction of Solar Acoustic Waves in Magnetic Regions
DOI: 10.1088/0004-637X/706/1/909 Bibcode: 2009ApJ...706..909C

Zhao, Hui; Liang, Zhi-Chao; Chou, Dean-Yi +2 more

Observed acoustic power in magnetic regions is lower than the quiet Sun because of absorption, emissivity reduction, and local suppression of solar acoustic waves in magnetic regions. In the previous studies, we have developed a method to measure the coefficients of absorption, emissivity reduction, and local suppression of sunspots. In this study…

2009 The Astrophysical Journal
SOHO 16
How the Solar Wind Ties to its Photospheric Origins
DOI: 10.1088/0004-637X/697/1/L28 Bibcode: 2009ApJ...697L..28L

McIntosh, Scott W.; Leamon, Robert J.

We present a new method of visualizing the solar photospheric magnetic field based on the "Magnetic Range of Influence" (MRoI). The MRoI is a simple realization of the magnetic environment in the photosphere, reflecting the distance required to balance the integrated magnetic field contained in any magnetogram pixel. It provides a new perspective …

2009 The Astrophysical Journal
SOHO 16
Coronal current sheet signatures during the 17 May 2002 CME-flare
DOI: 10.1051/0004-6361/200912229 Bibcode: 2009A&A...506..901A

Landini, F.; Poletto, G.; Aurass, H.

Context: The relation between current sheets (CSs) associated with flares, revealed by characteristic radio signatures, and current sheets associated with coronal mass ejections (CMEs), detected in coronal ultraviolet (UV) and white light data, has not been analyzed, yet.
Aims: We aim at establishing the relationship between CSs associated wit…

2009 Astronomy and Astrophysics
SOHO 16
Broad-band X-ray spectral evolution of GX 339-4 during a state transition
DOI: 10.1111/j.1365-2966.2008.14111.x Bibcode: 2009MNRAS.392..992D

Gehrels, N.; Homan, J.; van der Klis, M. +8 more

We report on X-ray and soft γ-ray observations of the black hole candidate GX 339-4 during its 2007 outburst, performed with the RXTE and INTEGRAL satellites. The hardness-intensity diagram of all RXTE/PCA data combined shows a q-shaped track similar to that observed in previous outbursts. The evolution in the diagram suggested that a transition f…

2009 Monthly Notices of the Royal Astronomical Society
INTEGRAL 16
Hubble Space Telescope NICMOS Polarization Observations of Three Edge-on Massive Young Stellar Objects
DOI: 10.1088/0004-637X/700/2/1488 Bibcode: 2009ApJ...700.1488S

Hines, Dean C.; Colgan, Sean W. J.; Burton, Michael G. +4 more

Massive young stellar objects (YSOs), like low-mass YSOs, appear to be surrounded by optically thick envelopes and/or disks and have regions, often bipolar, that are seen in polarized scattered light at near-infrared wavelengths. We are using the 0farcs2 spatial resolution of the Near Infrared Camera and Multi-Object Spectrometer (NICMOS) on Hubbl…

2009 The Astrophysical Journal
eHST 16
The Variable Star Population of the Globular Cluster B514 in the Andromeda Galaxy
DOI: 10.1088/0004-637X/704/2/L103 Bibcode: 2009ApJ...704L.103C

Kinemuchi, Karen; Marconi, Marcella; Pritzl, Barton J. +8 more

A rich harvest of RR Lyrae stars has been identified for the first time in B514, a metal-poor ([Fe/H] ~- 1.95 ± 0.10 dex) globular cluster (GC) of the Andromeda galaxy (M31), based on Hubble Space Telescope Wide Field Planetary Camera 2 and Advanced Camera for Surveys time-series observations. We have detected and derived periods for 89 RR Lyrae s…

2009 The Astrophysical Journal
eHST 16
Photometric and spectroscopic investigation of 2867 Steins, target of the Rosetta mission. Ground-based results prior to the Rosetta fly-by
DOI: 10.1051/0004-6361:200811340 Bibcode: 2009A&A...494L..29D

Barucci, M. A.; Fornasier, S.; Dotto, E. +8 more

Context: Rosetta is the cornerstone mission of ESA devoted to the study of minor bodies of the Solar System. During its journey to the comet 67P Churyumov-Gerasimenko, the main target, Rosetta also investigates two main belt asteroids, 2867 Steins (fly-by in September 2008) and 21 Lutetia (fly-by in July 2010).
Aims: In Spring 2008, we perform…

2009 Astronomy and Astrophysics
Rosetta 16