Spectroscopy of the Millennium Outburst and Recent Variability of the Yellow Hypergiant Rho Cassiopeiae

Details Spectroscopy of the Millennium Outburst and Recent Variability of the Yellow Hypergiant Rho Cassiopeiae Spectroscopy of the Millennium Outburst and Recent Variability of the Yellow Hypergiant Rho Cassiopeiae

2003-12-03

arxiv.org/abs/astro-ph/0312074v1

Astronomy and Astrophysics

Astrophysics

7 pages, 4 figures, To appear in A.S.P. Conference Series, IAU Symp. No. 219, 21-25 July 2003, Sydney, Australia. More Rho Cas

Scientific paper

In the summer and fall of 2000 the yellow hypergiant Rho Cassiopeiae dimmed by more than a visual magnitude, while its effective temperature decreased from \~7000 K to below 4000 K over ~200 d. We observed the highest mass-loss rate of ~5 % of the solar mass per year in a single stellar eruption so far (Lobel et al. 2003, ApJ, 583, 923). We determine from newly formed TiO bands a gas mass-loss rate of M_dot ~ 5.4 10^{-2} Msun/yr, which is of the same order of magnitude as has been proposed for the giant outbursts of the Luminous Blue Variable Eta Carinae. Over the past two years since the outburst event we observe a very prominent inverse P Cygni profile in Balmer H alpha. Strong Halpha emission has not before been observed in the hypergiant over this long period of time, signaling an unusual strong collapse of the upper hydrogen atmosphere, which we also observed in the months before the 2000 outburst. Since the brightness decrease of March 2003 we observe a transformation of the H alpha profile into a P Cygni profile, signaling a strong expansion of Rho Cas's upper atmosphere, which could possibly result in a new outburst event. High-resolution spectroscopic observations reveal that the lower photosphere rapidly expanded until May-June 2003. Very recent high-resolution observations of September 2003 show however that the photospheric absorption lines did not shift far blueward as observed in July 2000 before the strong brightness decrease of the outburst. The Fe I 5572 A is redshifted, signaling the collapse of the lower photosphere. A new strong brightness decrease by more than a magnitude in V for the fall and winter of 2003 is therefore not expected.

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