A dataset provided by the European Space Agency

Name GAS_DISC
Title GASEOUS CONTENT OF A FEW WELL-KNOWN BETA PICTORIS-LIKE STARS
URL

http://nida.esac.esa.int/nida-sl-tap/data?RETRIEVAL_TYPE=OBSERVATION&PRODUCT_LEVEL=ALL&obsno=404009040
DOI https://doi.org/10.5270/esa-e329t91
Author LECAVELIER, ALAIN
Description one of the major discoveries made by iras was the finding of disc of dust particles around a number of main sequence stars. these stars may not only be surrounded by dust particles, but also by gas discs. indeed, in the case of beta pictoris strong stable and variable redshifted absorption features are detected due to the absorption of the star light passing through a gaseous disc seen nearly edge on. after an extensive ground-based search of such gaseous discs, from a sample of about 50 stars, few revealed absorption features similar to beta pictoris ones (stable as well as variable). but the origin of this gas and the evolution of such discs are not well understood. the observations made in absorption however detect only the part of the disc just along the line of sight. the strength of the iso observations in the contrary is to sample the whole gas distribution around the star whatever the tilt of the disc on the line of sight is. the observations of the infrared emission lines will allow to determine the composition and eventually the ionization state of these gaseous component of the discs. since the composition is related to the history of the matter with n/c and n/o ratio or the proportion of these volatile elements compared to those of refractory. this will be check by measuring c/fe or o/fe ratio. the new information given by iso will allow to distinguish between primordial gas with cosmic characteristics and gas replenished by evaporating bodies. the observations of the stars proposed here will thus improve our knowledge of the possible presence of large bodies around stars.
Instrument LWS01 , SWS01 , SWS07
Temporal Coverage 1996-08-21T08:42:36Z/1997-06-10T15:06:48Z
Version 1.0
Mission Description The Infrared Space Observatory (ISO) was the worlds first true orbiting infrared observatory. Equipped with four highly-sophisticated and versatile scientific instruments, it was launched by Ariane in November 1995 and provided astronomers world-wide with a facility of unprecedented sensitivity and capabilities for a detailed exploration of the Universe at infrared wavelengths.
Creator Contact https://support.cosmos.esa.int/iso/
Date Published 1999-04-04T00:00:00Z
Last Update 2026-07-09
Keywords Infrared Space Observatory data, ESA ISO mission dataset, ISO infrared observations, mid-infrared astronomy data, far-infrared spectroscopy dataset, ISOCAM imaging data, ISOPHOT photometry data, SWS short wavelength spectrometer data, LWS long wavelength spectrometer data, infrared spectral line observations, infrared imaging survey data, dust emission infrared observations, star formation infrared dataset, interstellar medium spectroscopy data, polycyclic aromatic hydrocarbons PAH features data, active galactic nuclei infrared observations, circumstellar envelope infrared data, planetary nebula infrared spectroscopy, extragalactic infrared survey data, calibrated ISO data products, FITS files infrared astronomy, spectral energy distribution infrared data, continuum photometry dataset, infrared spectral cubes, flux-calibrated infrared maps, ESA ISO Data Archive, legacy infrared space mission dataset
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, LECAVELIER et al., 1999, 'GASEOUS CONTENT OF A FEW WELL-KNOWN BETA PICTORIS-LIKE STARS', 1.0, European Space Agency, https://doi.org/10.5270/esa-e329t91
Rights Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.