Search Publications

The acoustic low-degree modes of the Sun measured with 14 years of continuous GOLF & VIRGO measurements
DOI: 10.1088/1742-6596/271/1/012049 Bibcode: 2011JPhCS.271a2049G

García, R. A.; Mathur, S.; Jiménez, A. +3 more

The helioseismic Global Oscillation at Low Frequency (GOLF) and the Variability of solar Irradiance and Gravity Oscillations (VIRGO) instruments onboard SoHO, have been observing the Sun continuously for the last 14 years. In this preliminary work, we characterize the acoustic modes over the entire p-mode range in both, Doppler velocity and lumino…

2011 GONG-SoHO 24: A New Era of Seismology of the Sun and Solar-Like Stars
SOHO 13
Hubble Space Telescope study of resolved red giant stars in the outer halos of nearby dwarf starburst galaxies
DOI: 10.1051/0004-6361/201015881 Bibcode: 2011A&A...530A..23R

van der Marel, R. P.; Aloisi, A.; Annibali, F. +2 more

Context. Central starbursts in galaxies are an extreme example of ongoing galaxy evolution. The outer parts of galaxies contain a fossil record of galaxy formation and evolution processes in the more distant past. The characterization of resolved stellar populations allows one a detailed study of these topics.
Aims: We observed the outer part…

2011 Astronomy and Astrophysics
eHST 13
Suzaku Measurement of Electron and Magnetic Energy Densities in the East Lobe of the Giant Radio Galaxy DA 240
DOI: 10.1093/pasj/63.sp3.S947 Bibcode: 2011PASJ...63S.947I

Isobe, Naoki; Tashiro, Makoto S.; Seta, Hiromi

A careful analysis of the Suzaku data of the giant radio galaxy DA 240, of which the size is 1.48 Mpc, revealed diffuse X-ray emission associated with its east lobe. The diffuse X-ray spectrum was described with a simple power-law model with a photon index of $\Gamma$<…

2011 Publications of the Astronomical Society of Japan
Suzaku 13
Distinguishing post-AGB impostors in a sample of pre-main sequence stars
DOI: 10.1051/0004-6361/201015592 Bibcode: 2011A&A...526A..24V

Vieira, R. G.; Szczerba, R.; Stasińska, G. +2 more

Context. A sample of 27 sources, cataloged as pre-main sequence stars by the Pico dos Dias Survey (PDS), is analyzed to investigate a possible contamination by post-AGB stars. The far-infrared excess due to dust present in the circumstellar envelope is typical of both categories: young stars and objects that have already left the main sequence and…

2011 Astronomy and Astrophysics
AKARI ISO 13
Long-term evolution of the aerosol debris cloud produced by the 2009 impact on Jupiter
DOI: 10.1016/j.icarus.2011.03.015 Bibcode: 2011Icar..214..462S

Hueso, R.; Sánchez-Lavega, A.; Fletcher, L. N. +43 more

We present a study of the long-term evolution of the cloud of aerosols produced in the atmosphere of Jupiter by the impact of an object on 19 July 2009 (Sánchez-Lavega, A. et al. [2010]. Astrophys. J. 715, L155-L159). The work is based on images obtained during 5 months from the impact to 31 December 2009 taken in visible continuum wavelengths and…

2011 Icarus
eHST 12
Large-scale Shock-ionized and Photoionized Gas in M83: The Impact of Star Formation
DOI: 10.1088/0004-637X/731/1/45 Bibcode: 2011ApJ...731...45H

Mutchler, Max; McCarthy, Patrick J.; Blair, William P. +20 more

We investigate the ionization structure of the nebular gas in M83 using the line diagnostic diagram, [O III](5007 Å)/Hβ versus [S II](6716 Å+6731 Å)/Hα, with the newly available narrowband images from the Wide Field Camera 3 (WFC3) of the Hubble Space Telescope (HST). We produce the diagnostic diagram on a pixel-by-pixel (0farcs2 × 0farcs2) basis …

2011 The Astrophysical Journal
eHST 12
Velocity distributions of superthermal electrons fitted with a power law function in the magnetosheath: Cluster observations
DOI: 10.1029/2010JA016118 Bibcode: 2011JGRA..116.3224L

Zhang, Tielong; Wang, Shui; Lu, Quanming +3 more

Satellite observations have revealed that superthermal electrons in space plasma generally possess a power law distribution. In this paper, we utilize a power law function to model the omnidirectional differential fluxes of superthermal electrons observed by Cluster in the magnetosheath. By assuming an isotropic pitch angle distribution and perfor…

2011 Journal of Geophysical Research (Space Physics)
Cluster 12
Distances and stellar population properties for 12 elliptical galaxies
DOI: 10.1051/0004-6361/201015670 Bibcode: 2011A&A...534A..35C

Cantiello, M.; Capaccioli, M.; Brocato, E.


Aims: We use the surface brightness fluctuation (SBF) technique to derive the distances and analyse the radial behaviour of stellar populations in a sample of 12 elliptical galaxies. The data are I-band images collected with the FORS1 camera at the Very Large Telescope (VLT), drawn from the ESO archive. The main purpose of our analysis is to …

2011 Astronomy and Astrophysics
eHST 12
X-ray and optical properties of broad absorption line quasars in the Canada-France-Hawaii Telescope Legacy Survey
DOI: 10.1111/j.1365-2966.2010.18190.x Bibcode: 2011MNRAS.413.1013S

Stalin, C. S.; Petitjean, P.; Srianand, R.

We study the X-ray and optical properties of 16 broad absorption line (BAL) quasars detected in a ≈3 deg2 region common to the wide synoptic (W-1) component of the Canada-France-Hawaii Telescope Legacy Survey (CFHTLS) and the XMM Large Scale Structure Survey (XMM-LSS). The BAL fraction is found to be 10 per cent in the full sample, 7 pe…

2011 Monthly Notices of the Royal Astronomical Society
XMM-Newton 12
An X-Ray Spectroscopic Study of the Hot Interstellar Medium toward the Galactic Bulge
DOI: 10.1093/pasj/63.sp3.S889 Bibcode: 2011PASJ...63S.889H

Mitsuda, Kazuhisa; Yamasaki, Noriko Y.; Wang, Q. Daniel +5 more

We present a detailed spectroscopic study of the hot gas toward the galactic bulge along the 4U 1820 $-$ 303 sight line by a combination analysis of emission and absorption spectra. In addition to the absorption lines of O VII K

2011 Publications of the Astronomical Society of Japan
Suzaku 12