2017年4月
Star formation law in the Milky Way
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN
- ,
- 巻
- 69
- 号
- 2
- 記述言語
- 英語
- 掲載種別
- 研究論文(学術雑誌)
- DOI
- 10.1093/pasj/psw123
- 出版者・発行元
- OXFORD UNIV PRESS
The Schmidt law (SF law) in the Milky Way was investigated using 3D distribution maps of H II regions and HI and molecular (H-2) gases with spatial resolutions of similar to 1 kpc in the Galactic plane and a few tens of pc in the vertical direction. H II regions were shown to be distributed in a star-forming (SF) disk with nearly constant vertical full thickness 92 pc in spatial coincidence with the molecular gas disk. The vertically averaged volume star formation rate (SFR) rho(SFR) in the SF disk is related to the surface SFR Sigma(SFR) by rho(SFR)/[M-circle dot yr(-1) kpc(-3)] = 9.26 x Sigma(SFR)/[M-circle dot yr(-1) kpc(-2)]. The SF law fitted by a single power law of gas density in the form of Sigma(SFR) alpha rho SFR alpha rho(alpha)(gas) and alpha Sigma(beta)(gas) showed indices of alpha = 0.78 +/- 0.05 for rho H-2 and 2.15 +/- 0.08 for rho(total), and beta = 1.14 +/- 0.23 for Sigma(total), where rho and Sigma denote volume and surface densities, respectively. The star formation rate is shown to be directly related to the molecular gas, but indirectly to HI and total gas densities. The dependence of the SF law on the gaseous phase is explained by the phase transition theory between HI and H-2.
- リンク情報
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- DOI
- https://doi.org/10.1093/pasj/psw123
- Web of Science
- https://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=JSTA_CEL&SrcApp=J_Gate_JST&DestLinkType=FullRecord&KeyUT=WOS:000401118500005&DestApp=WOS_CPL
- Scopus
- https://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85019470443&origin=inward 本文へのリンクあり
- Scopus Citedby
- https://www.scopus.com/inward/citedby.uri?partnerID=HzOxMe3b&scp=85019470443&origin=inward
- ID情報
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- DOI : 10.1093/pasj/psw123
- ISSN : 0004-6264
- eISSN : 2053-051X
- SCOPUS ID : 85019470443
- Web of Science ID : WOS:000401118500005