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Discovery of hide-clumps of molecular hydrogen in the Owl nebula

Published online by Cambridge University Press:  06 October 2025

G. Ramos-Larios*
Affiliation:
Instituto de Astronomía y Meteorología, CUCEI, Universidad de Guadalajara, Mexico
M. A. Guerrero
Affiliation:
Instituto de Astrofsica de Andaluca, IAA-CSIC, Granada, Spain
J. A. Toalá
Affiliation:
Instituto de Radioastronomía y Astrofísica, UNAM, Morelia, Mich., Mexico
S. Akras
Affiliation:
Institute for Astronomy, Astrophysics, Space Applications and Remote Sensing, Penteli, Greece
X. Fang
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences, Beijing, China

Abstract

The recent acquisition of high-quality deep images of planetary nebulae (PNe) in world-class telescopes has allowed the detection for the first time of a wealth of small-scale morphological features and structures that highlight the complexity of their formation history and the physical processes modeling them. In this work we present the discovery of a series of clumps embedded within the ionized nebular shell of the evolved PN NGC 3587, the Owl Nebula, that had escaped previous detections. The multi-wavelength analysis provided by GEMINI, NOT and Aristarchos in the optical and CFHT and Spitzer infrared images indicates that these clumps are formed by denser and colder material, with a notable content of molecular H2.

Information

Type
Poster Paper
Copyright
© The Author(s), 2025. Published by Cambridge University Press on behalf of International Astronomical Union

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References

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