Co multi-line imaging of nearby galaxies
WebThe largest CO-mapping survey for nearby galaxies in the world, CO Multi-line Imaging of Nearby Galaxies (COMING; Sorai et al. 2024, 1 hereafter S19) was carried out using the … WebThe largest CO-mapping survey for nearby galaxies in the world, CO Multi-line Imaging of Nearby Galaxies (COMING; Sorai et al. 2024, 1 hereafter S19) was carried out using …
Co multi-line imaging of nearby galaxies
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WebMay 3, 2024 · Label-free evaluation and monitoring of living cell conditions or functions by means of chemical and/or physical sensors in a real-time manner are increasingly desired in the field of basic research of cells and clinical diagnosis. In order to perform multi-parametric analysis of living cells on a chip, we here developed a surface plasmon … WebCO Multi-line Imaging of Nearby Galaxies (COMING). VI. Radial variations in star formation efficiency. External Source. chorus. Document Type. Version of Record . …
Webplies that multiple lines (in particular in the 3 mm band where Δν/ν is highest) are covered in each observation. The study presented here does not intend to discuss the details of every detected line but instead present the data and highlight the rich chemistry provided by ALMA’s new capabilities, in the nearby starburst galaxy NGC 253. WebThe scatter of molecular gas surface density within each galaxy becomes larger by ∼30%, and at most by 120%. Indices of the spatially resolved Kennicutt–Schmidt relation by 12 …
WebIn this study, we present the results of 12 CO(J = 1-0), 13 CO(J = 1-0), and C 18 O(J = 1-0) simultaneous observations of the dwarf galaxy NGC 2976 conducted as a part of the CO Multi-line Imaging of Nearby Galaxies (COMING) project using the Nobeyama 45 m telescope. We investigated the properties of the molecular gas and star formation in … WebApr 1, 2014 · CO Multi-line Imaging of Nearby Galaxies (COMING). II. Transitions between atomic and molecular gas, diffuse and dense gas, gas and stars in the dwarf galaxy NGC 2976. Takuya Hatakeyama, N. Kuno, +17 authors N. Nakai
WebWe present the results of ^{12}CO(J = 1-0) and ^{13}CO(J = 1-0) simultaneous mappings toward the nearby barred spiral galaxy NGC 4303 as part of the CO Multi-line Imaging of Nearby Galaxies (COMING) project. Barred spiral galaxies often show lower star-formation efficiency (SFE) in their bar region compared to the spiral arms. In this paper, we …
WebJul 27, 2016 · 12 CO(J = 1 − 0) and 13 CO(J = 1 − 0) maps which are newly obtain ed by the CO Multi-line Imaging of Nearby Galaxies (COMING) project with the NRO 45-m telescope. NGC 2903 is a gas-rich galaxy seater dimensionsWebAbstract. The 12 CO (J = 1→0) velocity fields of a sample of 20 nearby spiral galaxies, selected from the CO Multi-line Imaging of Nearby Galaxies (COMING) legacy project of Nobeyama Radio Observatory, have been analyzed by Fourier decomposition to determine their basic kinematic properties, such as circular and noncircular velocities. On average, … seater dining butterfly table argosWebWe examined radial variations in molecular-gas based star formation efficiency (SFE), which is defined as star formation rate per unit molecular gas mass, for 80 galaxies selected … seater bench seat cushionsWebFeb 11, 2024 · We present variations of R2/1 and effects of the assumption that R2/1 is a constant in 24 nearby galaxies using 12CO data obtained with the Nobeyama 45 m … pubs of ancoatsWebDec 1, 2024 · PDF We present the results of $^{12}\\textrm{C}$$\\textrm{O}$(J = 1–0) and $^{13}\\textrm{C}$$\\textrm{O}$(J = 1–0) simultaneous mappings toward the... Find, read and cite all the research ... seater dining table amazonWebAbstract. While molecular gas mass is usually derived from 12 CO(J = 1-0)—the most fundamental line for exploring molecular gas—it is often derived from 12 CO(J = 2-1) … pubs of champaign posterWebJan 31, 2024 · We examined radial variations in molecular-gas based star formation efficiency (SFE), which is defined as star formation rate per unit molecular gas mass, for 80 galaxies selected from the CO Multi-line Imaging of Nearby Galaxies project (Sorai et al. 2024). The radial variations in SFE for individual galaxies are typically a factor of 2 -- 3, … seater bed