Eta Carinae's Dusty Homunculus Nebula from Near-infrared to Submillimeter Wavelengths: Mass, Composition, and Evidence for Fading Opacity
Artikel i vetenskaplig tidskrift, 2017

Infrared observations of the dusty, massive Homunculus Nebula around the luminous blue variable eta Carinae are crucial to characterize the mass-loss history and help constrain the mechanisms leading to the great eruption. We present the 2.4-670 mu m spectral energy distribution, constructed from legacy Infrared Space Observatory observations and new spectroscopy obtained with the Herschel Space Observatory. Using radiative transfer modeling, we find that the two best-fit dust models yield compositions that are consistent with CNO-processed material, with iron, pyroxene and other metal-rich silicates, corundum, and magnesium-iron sulfide in common. Spherical corundum grains are supported by the good match to a narrow 20.2 mu m feature. Our preferred model contains nitrides AlN and Si3N4 in low abundances. Dust masses range from 0.25 to 0.44 M-circle dot, but M-tot. 45M(circle dot) in both cases, due to an expected high Fe gas-to-dust ratio. The bulk of dust is within a 5 '' x 7 '' central region. An additional compact feature is detected at 390 mu m. We obtain L-IR = 2.96 x 10(6) L-circle dot, a 25% decline from an average of mid-IR photometric levels observed in 1971-1977. This indicates a reduction in circumstellar extinction in conjunction with an increase in visual brightness, allowing 25%-40% of optical and UV radiation to escape from the central source. We also present an analysis of (CO)-C-12 and (CO)-C-13 J = 5-4 through 9-8 lines, showing that the abundances are consistent with expectations for CNO-processed material. The [C-12 II] line is detected in absorption, which we suspect originates in foreground material at very low excitation temperatures.

dust

stars: mass-loss

stars: massive

stars: individual (eta Carinae)

circumstellar matter

extinction

Författare

P. W. Morris

CalTech

T. R. Gull

NASA Goddard Space Flight Center

D. J. Hillier

University of Pittsburgh

M. J. Barlow

University College London (UCL)

P. Royer

KU Leuven

K. Nielsen

Catholic University of America

John H Black

Astronomi och plasmafysik

B. Swinyard

Rutherford Appleton Laboratory

Astrophysical Journal

0004-637X (ISSN) 1538-4357 (eISSN)

Vol. 842 2 Article no. 79 - 79

Ämneskategorier

Astronomi, astrofysik och kosmologi

Fundament

Grundläggande vetenskaper

Infrastruktur

Onsala rymdobservatorium

DOI

10.3847/1538-4357/aa71b3