A high-resolution image of the inner shell of the P Cygni nebula in the infrared [Fe ii] line
Carmelo Arcidiacono(Arcetri Astrophysical Observatory), D. Paris(Astronomical Observatory of Rome), Craig Kulesa(University of Arizona), Enrico Pinna(Arcetri Astrophysical Observatory), Runa Briguglio, Lorenzo Busoni(Arcetri Astrophysical Observatory), Marco Xompero(Arcetri Astrophysical Observatory), Roberto Ragazzoni(Osservatorio Astronomico di Padova), P. Di Marcantonio, Fernando Quirós-Pacheco(Arcetri Astrophysical Observatory), M. Franchini(Trieste Astronomical Observatory), K. Boutsia(Las Campanas Observatory), D. W. McCarthy(University of Arizona), C. Morossi(Trieste Astronomical Observatory)
Cited by 3
Related Papers
CHARACTERISTICS OF PLANETARY CANDIDATES OBSERVED BY<i>KEPLER</i>. II. ANALYSIS OF THE FIRST FOUR MONTHS OF DATA
|The Astrophysical Journal|2011|1.1k
Terahertz Spectroscopy for Astronomy: From Comets to Cosmology
|IEEE Transactions on Terahertz Science and Technology|2011|217
THE HIGH ALBEDO OF THE HOT JUPITER KEPLER-7 b
|The Astrophysical Journal Letters|2011|161
The PLATO mission
|Experimental Astronomy|2025|155
An Imaging Survey for Extrasolar Planets around 45 Close, Young Stars with the Simultaneous Differential Imager at the Very Large Telescope and MMT
|The Astrophysical Journal Supplement Series|2007|152