Results 81 to 90 of about 52,795 (103)
Human breathing perception system based on Wi-Fi subcarrier mutual information
The unpredictable environmental changes cause large fluctuations in Wi-Fi signals, and it is difficult to quantify the static and behaviorally-aware dynamic components in the subcarriers, so it is not possible to accurately portray the fluctuating form ...
Ying LIU, Mengyuan HU, Zhihong QIAN
doaj
Editorial Status Update of OJAP
Zhongxiang Shen
doaj +1 more source
Herschelimages of NGC 6720: H2formation on dust grains [PDF]
Herschel PACS and SPIRE images have been obtained of NGC 6720 (the Ring nebula). This is an evolved planetary nebula with a central star that is currently on the cooling track, due to which the outer parts of the nebula are recombining. From the PACS and
M J Barlow, B Sibthorpe, Toshiya Ueta
exaly +4 more sources
WEAVE imaging spectroscopy of NGC 6720: an iron bar in the Ring [PDF]
We present spatially resolved spectroscopic observations of the planetary nebula NGC 6720, the Ring Nebula, taken during the science verification phase of WEAVE, a new instrument mounted on the William Herschel Telescope on La Palma.
P J Storey, R Wesson, J E Drew
exaly +6 more sources
The nucleotide sequence of the 3′ end of the nifU coding sequence, the complete coding sequence of nifH and a substantial part of the 5′ end of nifD coding sequence from Nostoc 6720 is presented.
Stephen J Temple, Peter J Lea
exaly +1 more source
A 21-kDa novel polypeptide which possesses characteristics normally considered to be diagnostic of the calmodulin present in eukaryotic cells was isolated from the cyanobacterium Nostoc sp. PCC 6720.
Peter J Lea, Lea Peter J
exaly +1 more source
JWST observations of the Ring Nebula (NGC 6720) – II. PAH emission [PDF]
Polycyclic aromatic hydrocarbons (PAHs) and carbonaceous dust have been observed in clumpy circumstellar environments, yet their formation and evolutionary pathways in such environments remain elusive.
E Peeters, J Cami, M J Barlow
exaly +3 more sources
The Structure of the Molecular Envelope of the Ring Nebula (NGC 6720)
We present the first interferometric imaging of molecular line emission from the Ring Nebula,NGC 6720, in the form of Submillimeter Array (SMA) observations of C O J = 2 → 1 emission.
Joel H Kästner +2 more
exaly +2 more sources
JWST observations of the Ring Nebula (NGC 6720): I. Imaging of the rings, globules, and arcs [PDF]
We present JWST images of the well-known planetary nebula NGC 6720 (the Ring Nebula), covering wavelengths from 1.6 to 25 m. The bright shell is strongly fragmented with some 20 000 dense globules, bright in H2, with a characteristic diameter of 0.2 ...
R Wesson, M Matsuura, P J Kavanagh
exaly +1 more source

