On the relation between the mysterious 21 μm emission feature of post-asymptotic giant branch stars and their mass-loss rates

Journal Article · Fri Jul 01 04:00:00 EDT 2016 · Astrophysical Journal

DOI:https://doi.org/10.3847/0004-637X/825/1/68· OSTI ID:22868931

Mishra, Ajay; Li, Aigen ^[1]

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1. Department of Physics and Astronomy, University of Missouri, Columbia, MO 65211 (United States)

Over two decades ago, a prominent, mysterious emission band peaking at ∼20.1 μm was serendipitously detected in four preplanetary nebulae (PPNe; also known as “protoplanetary nebulae”). To date, this spectral feature, designated as the “21 μm” feature, has been seen in 27 carbon-rich PPNe in the Milky Way and the Magellanic Clouds. The nature of its carriers remains unknown although many candidate materials have been proposed. The 21 μm sources also exhibit an equally mysterious, unidentified emission feature peaking at 30 μm. While the 21 μm feature is exclusively seen in PPNe, a short-lived evolutionary stage between the end of the asymptotic giant branch (AGB) and planetary nebula (PN) phases, the 30 μm feature is more commonly observed in all stages of stellar evolution from the AGB through PPN to PN phases. We derive the stellar mass-loss rates ( M-dot ) of these sources from their infrared (IR) emission, using the “2-DUST” radiative transfer code for axisymmetric dusty systems which allows one to distinguish the mass-loss rates of the AGB phase ( M-dot {sub AGB}) from that of the superwind ( M-dot {sub SW}) phase. We examine the correlation between M-dot {sub AGB} or M-dot {sub SW} and the fluxes emitted from the 21 and 30 μm features. We find that both features tend to correlate with M-dot {sub AGB}, suggesting that their carriers are probably formed in the AGB phase. The nondetection of the 21 μm feature in AGB stars suggests that, unlike the 30 μm feature, the excitation of the carriers of the 21 μm feature may require ultraviolet photons which are available in PPNe but not in AGB stars.

• OSTI ID: 22868931
• Journal Information: Astrophysical Journal, Journal Name: Astrophysical Journal Journal Issue: 1 Vol. 825; ISSN ASJOAB; ISSN 0004-637X
• Country of Publication: United States
• Language: English

Related Subjects

79 ASTRONOMY AND ASTROPHYSICS
ASYMPTOTIC SOLUTIONS
AXIAL SYMMETRY
COSMIC DUST
EXCITATION
GIANT STARS
MAGELLANIC CLOUDS
MASS TRANSFER
MILKY WAY
PLANETARY NEBULAE
PROTOPLANETS
RADIANT HEAT TRANSFER
STAR EVOLUTION
STELLAR WINDS
ULTRAVIOLET RADIATION