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Mercury in the HgMn stars chi Lupi and HR 7775

Title: Mercury in the HgMn stars chi Lupi and HR 7775
Authors: Proffitt, CR; Brage, Tomas; Leckrone, DS; Wahlgren, Glenn; Brandt, JC; Sansonetti, CJ; Reader, J; Johansson, Sveneric
Source: Astrophysical Journal; 512(2), pp 942-960 (1999) ; ISSN: 0004-637X
Publisher Information: American Astronomical Society
Publication Year: 1999
Collection: Lund University Publications (LUP)
Subject Terms: Astronomy; Astrophysics and Cosmology; HR 7775); stars : peculiar; stars : individual (chi Lupi; diffusion; stars : abundances
Description: Observations of mercury lines in the HgMn stars chi Lupi and HR 7775 made with the Hubble Space Telescope Goddard High Resolution Spectrograph are presented and analyzed. In chi Lupi we find that all observed lines are consistent with the same isotopic mixture (essentially pure (204)Hg). Strong ionization anomalies are present, with UV Hg I lines being too weak and Hg III lines too strong for the abundance derived from lines of the majority ionization state, Hg rr. Observations of mercury in I;IR 7775 show less extreme isotope and ionization anomalies. We find that the ionization anomaly in the Hg I resonance lines can be plausibly explained as a non-LTE effect, but the same non-LTE calculations show that the Hg III ionization anomaly in chi Lupi cannot be explained in this way. Radiative force calculations show that the observed mercury abundance cannot be supported in the atmosphere by the radiative forces alone. We suggest that weak mixing brings mercury into the line-forming region from below the photosphere, while a wind of order 10(-14) M. yr(-1) supports a cloud of Hg III at very small optical depths.
Document Type: article in journal/newspaper
Language: English
Relation: https://lup.lub.lu.se/record/3919505; http://dx.doi.org/10.1086/306783; wos:000079809000036; scopus:0033585746
DOI: 10.1086/306783
Availability: https://lup.lub.lu.se/record/3919505; https://doi.org/10.1086/306783
Accession Number: edsbas.2EB6B9CD
Database: BASE