The EURONEAR_Release1 catalog contains 1544 positions of 155 Near-Earth Asteroids, obtained between 2006 and 2008. (2 data files).
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Near Earth Asteroids positions (Birlan+, 2010)Birlan, M. et al.112009
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Near-infrared study of the stellar population of Sh2-152
Context. The discovery of new massive star clusters and massive stellar populations in previously known clusters in our Galaxy by means of infrared studies has changed our view of the Milky Way from an inactive to an active star-forming machine. Within this scenario, we present a near-infrared spectrophotometric study of the stellar content of the
Ramírez-Alegría, S. et al.Fecha de publicación:
112011 -
Near-IR variability properties of a selected sample of AGB stars
We present the results of a near-infrared monitoring programme of a selected sample of stars, initially suspected to be Mira variables and OH/IR stars, covering more than a decade of observations. The objects monitored cover the typical range of IRAS colours shown by O-rich stars on the asymptotic giant branch and show a surprisingly large
Jiménez-Esteban, F. M. et al.Fecha de publicación:
112006 -
Neutron-capture Element Abundances in Magellanic Cloud Planetary Nebulae
We present near-infrared spectra of 10 planetary nebulae (PNe) in the Large and Small Magellanic Clouds (LMC and SMC), acquired with the FIRE and GNIRS spectrometers on the 6.5 m Baade and 8.1 m Gemini South Telescopes, respectively. We detect Se and/or Kr emission lines in eight of these objects, the first detections of n-capture elements in
Mashburn, A. L. et al.Fecha de publicación:
112016 -
New candidate planetary nebulae in M 81
A 34'x34' field centred on the spiral galaxy M 81 has been searched for emission-line objects using the prime focus wide field camera (WFC) of the 2.54 m Isaac Newton Telescope (La Palma, Spain). A total of 171 candidate planetary nebulae (PNe) are found, 54 of which are in common with the ones detected by Jacoby et al. (1989). The behaviour of PNe
Magrini, L. et al.Fecha de publicación:
112001 -
New clues on outburst mechanisms and improved spectroscopic elements of the black hole binary V4641 Sagittarii*
We present spectroscopic observations of the black hole binary V4641 Sagittarii, obtained between 2004 July 4 and 2005 March 28, which cover the minor outburst of the star in early 2004 July and quiescence variations on 19 nights scattered over six months. During the outburst, the star peaked approximately 3 mag brighter than usual, and our spectra
Lindstrøm, C. et al.Fecha de publicación:
112005