R Coronae Borealis at the 2003 Light Minimum

Abstract

High-resolution optical spectra of R CrB obtained in 2003 March is discussed. The 2003 spectra are compared with the extensive collection of spectra from the 1995-1996 minimum. Spectroscopic features common to the two minima include sharp emission lines of neutral and singly-ionized atoms, broad emission lines including He {\sc i}, [N {\sc ii}] 6583 Å, Na D, and Ca {\sc ii} H & K lines, and blueshifted aborption lines of Na D, and K {\sc i} resonance lines. Prominent differences between the 2003 and 1995-96 spectra are seen. The 2003 profiles of Na D, Ca II H & K are fit by a single Gaussian but in 1995-1996 two Gaussians separated by about 200 km s${}^{-1}$ were required. However, the He {\sc i} broad emission lines are fit by a single Gaussian at all times; the emitting He and Na-Ca atoms are probably not colocated. The C${}_2$ Phillips 2-0 lines are detected as sharp absorption lines in 2003 indicating presence of gas at 1300 K.The 2003 spectra show C {\sc i} sharp emission lines at minimum light with a velocity changing in five days by about 20 km s${}^{-1}$ when the velocity of `metal' sharp lines is unchanged; the C {\sc i} emission may arise from shock-heated gas. Spectra at maximum shows extended blue wings to strong lines with the extension dependent on a line's lower excitation potential a signature of stellar wind. Changes in the cores of the resonance lines of Al {\sc i} and Na D and the Ca {\sc ii} IR lines suggest complex flow patterns near the photosphere. The spectroscopic differences at the two mimima show the importance of continued scrutiny of the declines of R CrB.

14 pages (including 20 figures), accepted for publication in MNRAS

References in corpus (5)

• The 1995-1996 Decline of R Coronae Borealis - High Resolution Optical Spectroscopy
• Winds in R Coronae Borealis Stars
• First detection of dust clouds around R CrB variable stars
• High-resolution spectroscopy of V854 Cen in decline - Absorption and emission lines of C_2 molecules
• R Coronae Borealis Stars at Minimum Light -- UW Cen

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• Variable Winds and Dust Formation in R Coronae Borealis Stars
• The evolutionary status of the semiregular variable QYSge
• Do Hydrogen-deficient Carbon Stars have Winds?
• The variable V381 Lac and its possible connection with the R CrB phenomenon
• High-resolution spectroscopy of the R Coronae Borealis and Other Hydrogen Deficient Stars
• High-resolution optical spectroscopy of the R Coronae Borealis star V532 Ophiuchi at maximum light
• Spectropolarimetry of R Coronae Borealis in 1998--2003: Discovery of Transient Polarization at Maximum Brightness