Atomic hydrogen in AGB circumstellar environments. A case study : X Her
hal.structure.identifier | Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique [LERMA] | |
hal.structure.identifier | Laboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB] | |
hal.structure.identifier | Observatoire aquitain des sciences de l'univers [OASU] | |
hal.structure.identifier | Laboratoire d'Astrophysique de Bordeaux [Pessac] [LAB] | |
dc.contributor.author | GARDAN, E. | |
hal.structure.identifier | Galaxies, Etoiles, Physique, Instrumentation [GEPI] | |
dc.contributor.author | GERARD, E. | |
hal.structure.identifier | Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique [LERMA] | |
dc.contributor.author | LE BERTRE, T. | |
dc.date.issued | 2006 | |
dc.identifier.issn | 0035-8711 | |
dc.description.abstractEn | We report the detection of the Hi line at 21 cm from the circumstellar shell around the AGB star X Her using the position-switching technique with the Nan¸cay RadioTelescope. At the star position the line shows 2 components: (i) a broad one (FWHM 13 kms?1) centered at ?72.2 kms?1, and (ii) a narrow one (FWHM 4 kms?1) centered at ?70.6 kms?1. Our map shows that the source associated to the broad component is asymmetric with material flowing preferentially towards the North-East. This source extends to 10? ( 0.4 pc) from the star in that direction. On the other hand, the narrow component is detected only at the star position and indicates mate-rial flowing away from the observer. The total mass of atomic hydrogen is 6.5 10?3 M? which, within a factor 2, agrees with the estimate obtained from IRAS data at 60 ?m | |
dc.language.iso | en | |
dc.publisher | Oxford University Press (OUP): Policy P - Oxford Open Option A | |
dc.subject.en | stars: late- type | |
dc.subject.en | stars: mass-loss | |
dc.subject.en | (ISM:) planetary nebulae: general | |
dc.subject.en | radio lines: stars | |
dc.subject.en | stars: AGB and post-AGB | |
dc.subject.en | (stars:) circumstellar matter | |
dc.subject.en | radio lines: stars. | |
dc.title.en | Atomic hydrogen in AGB circumstellar environments. A case study : X Her | |
dc.type | Article de revue | |
dc.subject.hal | Physique [physics]/Astrophysique [astro-ph]/Cosmologie et astrophysique extra-galactique [astro-ph.CO] | |
dc.subject.hal | Planète et Univers [physics]/Astrophysique [astro-ph] | |
bordeaux.journal | Monthly Notices of the Royal Astronomical Society | |
bordeaux.page | 245-254 | |
bordeaux.volume | 365 | |
bordeaux.peerReviewed | oui | |
hal.identifier | hal-00023313 | |
hal.version | 1 | |
hal.popular | non | |
hal.audience | Non spécifiée | |
hal.origin.link | https://hal.archives-ouvertes.fr//hal-00023313v1 | |
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