Search Publications

The infrared Hourglass cluster in M8*
DOI: 10.1111/j.1365-2966.2005.09829.x Bibcode: 2006MNRAS.366..739A

Maíz Apellániz, J.; Barbá, R. H.; Rubio, M. +2 more

A detailed study of the Hourglass nebula in the M8 star-forming region is presented. The study is mainly based on recent subarcsec-resolution JHKs images taken at Las Campanas Observatory and complemented with archival Hubble Space Telescope (HST) images and long-slit spectroscopy retrieved from the European Southern Observatory Archive…

2006 Monthly Notices of the Royal Astronomical Society
eHST 48
3D spectroscopy with VLT/GIRAFFE. II. Are luminous compact galaxies merger remnants?
DOI: 10.1051/0004-6361:20054218 Bibcode: 2006A&A...455..119P

Östlin, G.; Flores, H.; Hammer, F. +2 more

Luminous Compact Galaxies (LCGs) are enigmatic sources in many aspects. They can reach the luminosity of the Milky Way within a radius of only a few kpc. They also represent one of the most rapidly evolving populations of galaxies since they represent up to 1/5 of the luminous galaxies at redshift z= 0.7, while being almost absent in the local Uni…

2006 Astronomy and Astrophysics
eHST 48
How extreme are the Wolf-Rayet clusters in NGC3125?*
DOI: 10.1111/j.1365-2966.2006.10245.x Bibcode: 2006MNRAS.368.1822H

Crowther, P. A.; Hadfield, L. J.

We reinvestigate the massive stellar content of the irregular dwarf galaxy NGC3125 (Tol 3) using Very Large Telescope (VLT)/FORS1 imaging and spectroscopy, plus archival VLT/ISAAC, Hubble Space Telescope (HST)/FOC and HST/STIS data sets. FORS1 narrow-band imaging confirms that the NGC3125-A and -B knots represent the primary sites of Wolf-Rayet (W…

2006 Monthly Notices of the Royal Astronomical Society
eHST 48
Two years of INTEGRAL monitoring of the soft gamma-ray repeater SGR 1806-20: from quiescence to frenzy
DOI: 10.1051/0004-6361:20053648 Bibcode: 2006A&A...445..313G

Hurley, K.; Sunyaev, R.; Götz, D. +16 more

SGR 1806-20 has been observed for more than 2 years with the INTEGRAL satellite. In this period the source went from a quiescent state into a very active one culminating in a giant flare on December 27, 2004. Here we report on the properties of all the short bursts detected with INTEGRAL before the giant flare. We derive their number-intensity dis…

2006 Astronomy and Astrophysics
INTEGRAL 48
Deep Chandra and Multicolor HST Follow-up of the Jets in Two Powerful Radio Quasars
DOI: 10.1086/500526 Bibcode: 2006ApJ...641..717S

Maraschi, L.; Cheung, C. C.; Tavecchio, F. +5 more

We present deep (70-80 ks) Chandra and multicolor HST ACS images of two jets hosted by the powerful quasars 1136-135 and 1150+497, together with new radio observations. The sources have an FR II morphology and were selected from our previous X-ray and optical jet survey for detailed follow-up aimed at obtaining better constraints on the jet multiw…

2006 The Astrophysical Journal
eHST 48
A statistical comparison of solar wind sources of moderate and intense geomagnetic storms at solar minimum and maximum
DOI: 10.1029/2005JA011065 Bibcode: 2006JGRA..111.1104Z

Liemohn, Michael W.; Thomsen, Michelle F.; Weygand, James M. +3 more

Superposed epoch analyses of 549 storms are performed to make a comparison of solar wind features of geomagnetic storm events at solar minimum (July 1974 to June 1977; July 1984 to June 1987; July 1994 to June 1997) and solar maximum (January 1979 to December 1981; January 1989 to December 1991; July 1999 to June 2002). In this study, geomagnetic …

2006 Journal of Geophysical Research (Space Physics)
Ulysses 48
Large-scale source regions of earth-directed coronal mass ejections
DOI: 10.1051/0004-6361:20053536 Bibcode: 2006A&A...445.1133Z

Zhang, J.; Wang, J. X.; Zhou, G. P.

Based on SOHO/MDI, EIT, Yohkoh/SXT, Hα, and other relevant observations, we analyzed all the earth-directed halo coronal mass ejections (CMEs) in the interval from Mar. 1997 to Dec. 2003. A total of 288 earth-directed CMEs were studied and their associated surface activity events identified. Unlike the previous studies that often attributed a surf…

2006 Astronomy and Astrophysics
SOHO 48
Simultaneous Ultraviolet and X-Ray Observations of the Seyfert Galaxy NGC 4151. II. Physical Conditions in the UV Absorbers
DOI: 10.1086/508629 Bibcode: 2006ApJS..167..161K

Gull, T. R.; Kriss, G. A.; Turner, T. J. +8 more

We present a detailed analysis, including photoionization modeling, of the intrinsic absorption in the Seyfert 1 galaxy NGC 4151 using ultraviolet (UV) spectra from the Hubble Space Telescope Space Telescope Imaging Spectrograph and the Far Ultraviolet Spectrographic Explorer obtained 2002 May as part of a set of contemporaneous observations that …

2006 The Astrophysical Journal Supplement Series
IUE eHST 48
Electron oscillations in the induced martian magnetosphere
DOI: 10.1016/j.icarus.2005.10.033 Bibcode: 2006Icar..182..360W

Coates, A. J.; Kallio, E.; Fedorov, A. +42 more

The Analyzer of Space Plasmas and Energetic Atoms (ASPERA-3) experiment flown on the Mars Express (MEX) spacecraft includes the Electron Spectrometer (ELS) as part of its complement. The ELS instrument measures the differential electron flux spectrum in a 128-level logarithmic energy sweep within a time period of 4 s. The orbital path of MEX trave…

2006 Icarus
MEx 48
First ENA observations at Mars: ENA emissions from the martian upper atmosphere
DOI: 10.1016/j.icarus.2005.09.019 Bibcode: 2006Icar..182..424F

Coates, A. J.; Kallio, E.; Fedorov, A. +44 more

The neutral particle detector (NPD) on board Mars Express has observed energetic neutral atoms (ENAs) from a broad region on the dayside of the martian upper atmosphere. We show one such example for which the observation was conducted at an altitude of 570 km, just above the induced magnetosphere boundary (IMB). The time of flight spectra of these…

2006 Icarus
MEx 48