Search Results - "Bohigas, J"
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An analytical model for the evolution of the coldest component of the Boomerang Nebula
Published in Monthly notices of the Royal Astronomical Society (01-04-2017)“…The most striking feature of the Boomerang Nebula is a large nearly spherical cloud where the temperature is close to 2 K. At its inner and outer boundaries,…”
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Balmer ratios, the abundance discrepancy factor and a two temperature component nebula
Published in Monthly notices of the Royal Astronomical Society (21-10-2015)“…Large values of the Hα/Hβ line ratio are preferentially found in planetary nebulae (PNe) with large abundance discrepancy factors (ADFs) for O+2. This…”
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Echelle spectroscopy and photoionization modelling of the entire planetary nebula NGC 6210
Published in Monthly notices of the Royal Astronomical Society (11-02-2015)“…High-resolution spectroscopy of NGC 6210, show that recombination line abundances of O+2 and Ne+2 are two to three times larger than forbidden line abundances,…”
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The Expanding Nebular Remnant of the Recurrent Nova RS Ophiuchi (2006). II. Modeling of Combined Hubble Space Telescope Imaging and Ground-based Spectroscopy
Published in The Astrophysical journal (01-10-2009)“…We report Hubble Space Telescope (HST) imaging, obtained 155 and 449 days after the 2006 outburst of the recurrent nova RS Ophiuchi, together with ground-based…”
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Imaging study of NGC 3372, the Carina nebula — II. Evidence of activity in the complex Trumpler 14/Car I photodissociation region
Published in Monthly notices of the Royal Astronomical Society (01-04-2006)“…We present the results of an imaging survey, from the optical to the mid-infrared, of the dark cloud associated with Car I, a dense cloud that is subject to an…”
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Photoionization Models Applied to Planetary Nebulae
Published in The Astrophysical journal (20-02-2008)“…Good to excellent photoionization models based on the Cloudy code (from Ferland and coworkers) were obtained for 13 out of 19 spectra of planetary nebulae…”
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Spectrophotometry of RS Oph during the nebular phase
Published in Monthly notices of the Royal Astronomical Society (01-06-1989)“…We present blue-wavelength spectroscopic observations of RS Oph, 201 day after the 1985 outburst. An analysis of the TiO bands indicates a spectral type M4III…”
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Simultaneous Multiwavelength Observations of Dwarf Novae. I. SU Ursae Majoris: Minihumps at a Minioutburst?
Published in The Astrophysical journal (01-08-1996)Get full text
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Possible detection of an old bipolar shell associated with Carinae
Published in Monthly notices of the Royal Astronomical Society (21-02-2000)Get full text
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Possible detection of an old bipolar shell associated with η Carinae
Published in Monthly notices of the Royal Astronomical Society (21-02-2000)“…Continuum-subtracted dereddened images in the light of several atomic lines show the presence of an extended bipolar nebula surrounding η Carinae with size…”
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The Warm Interstellar Medium around the Cygnus Loop
Published in The Astrophysical journal (10-06-1999)Get full text
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The warm interstellar medium around the Cygnus Loop
Published 20-11-1998“…Observations of the oxygen lines [OII]3729 and [OIII]5007 in the medium immediately beyond the Cygnus Loop supernova remnant were carried out with the scanning…”
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The Expanding Nebular Remnant of the Recurrent Nova RS Ophiuchi (2006): II. Modeling of Combined Hubble Space Telescope Imaging and Ground-based Spectroscopy
Published 24-08-2009“…Astrophysical Journal 703 (2009) 1955-1963 We report Hubble Space Telescope imaging, obtained 155 and 449 days after the 2006 outburst of the recurrent nova RS…”
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