Title A Mysterious Ring in Dark Space?
Authors Zhang, Wei
Yang, Fan
Wu, Hong
Wu, Chaojian
Zou, Hu
Zhang, Tianmeng
Zhou, Xu
Lei, Fengjie
Jin, Junjie
Zhou, Zhimin
Nie, Jundan
Ma, Jun
Wang, Jiali
Affiliation Chinese Acad Sci, Key Lab Opt Astron, Natl Astron Observ, Beijing 100101, Peoples R China
Peking Univ, Sch Phys, Dept Astron, Beijing 100871, Peoples R China
Keywords PLANETARY-NEBULAE
MILKY-WAY
EMISSION
GALAXY
IRAS
EXTINCTION
EXPLORER
CIRRUS
CLOUD
SYSTEM
Issue Date Apr-2020
Publisher ASTROPHYSICAL JOURNAL
Abstract We report the discovery of a low-surface-brightness (27.42 mag arcsec(-2) in g band) nebula, which has a ring-like shape in the Beijing-Arizona Sky Survey (BASS). Positive detections have been found in multiband data from far-ultraviolet to far-infrared, except the z band from BASS and W1, W2 from the Wide-field Infrared Survey Explorer. The reddening of the nebula E(B - V) similar to 0.02 mag is estimated from Infrared Astronomical Satellite (IRAS) 100 mu m intensity and H i column density. With the help of the 3D reddening map from Pan-STARRS 1, the Two Micron All Sky Survey, and Gaia, the distance to the nebula of about 500 pc from Earth is derived. Such a low-surface-brightness nebula whose energy can be interpreted by the diffuse Galactic light could account for the optical counterpart of the infrared cirrus, which was detected by IRAS more than 30 yr ago. The ring-like structure might be the ultimate phase of an evolved planetary nebula, while the central white dwarf star has been ejected from the nebula for an unclear reason. On the other hand, the ring structure being a superposition of two close filaments might be another reasonable explanation. Considering the lack of spectroscopic data and uncertainty in the distance measurement, these interpretations need to be checked by future observations.
URI http://hdl.handle.net/20.500.11897/588620
ISSN 0004-637X
DOI 10.3847/1538-4357/ab7c5a
Indexed SCI(E)
Scopus
Appears in Collections: 物理学院

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