Cloud formation in the atomic and molecular phase: H I self absorption (HISA) towards a giant molecular filament
Molecular clouds form from the atomic phase of the interstellar medium. However, characterizing the transition between the atomic and the molecular interstellar medium (ISM) is a complex observational task. Here we address cloud formation processes by combining H I self absorption (HISA) with molecu...
Gespeichert in:
| Hauptverfasser: | , , , , , , , , , , , , , , , , , , , , , , |
|---|---|
| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
February 2020
|
| In: |
Astronomy and astrophysics
Year: 2020, Jahrgang: 634 |
| ISSN: | 1432-0746 |
| DOI: | 10.1051/0004-6361/201935866 |
| Online-Zugang: | Verlag, lizenzpflichtig, Volltext: https://dx.doi.org/10.1051/0004-6361/201935866 Verlag, lizenzpflichtig, Volltext: https://www.aanda.org/articles/aa/abs/2020/02/aa35866-19/aa35866-19.html 
|
| Verfasserangaben: | Y. Wang, S. Bihr, H. Beuther, M.R. Rugel, J.D. Soler, J. Ott, J. Kainulainen, N. Schneider, R.S. Klessen, S.C.O. Glover, N.M. McClure-Griffiths, P.F. Goldsmith, K.G. Johnston, K.M. Menten, S. Ragan, L.D. Anderson, J.S. Urquhart, H. Linz, N. Roy, R.J. Smith, F. Bigiel, T. Henning, and S.N. Longmore |
MARC
| LEADER | 00000caa a2200000 c 4500 | ||
|---|---|---|---|
| 001 | 1745593896 | ||
| 003 | DE-627 | ||
| 005 | 20220819084112.0 | ||
| 007 | cr uuu---uuuuu | ||
| 008 | 210125s2020 xx |||||o 00| ||eng c | ||
| 024 | 7 | |a 10.1051/0004-6361/201935866 |2 doi | |
| 035 | |a (DE-627)1745593896 | ||
| 035 | |a (DE-599)KXP1745593896 | ||
| 035 | |a (OCoLC)1341389300 | ||
| 040 | |a DE-627 |b ger |c DE-627 |e rda | ||
| 041 | |a eng | ||
| 084 | |a 29 |2 sdnb | ||
| 100 | 1 | |a Wang, Yuan |e VerfasserIn |0 (DE-588)1188747975 |0 (DE-627)1667656899 |4 aut | |
| 245 | 1 | 0 | |a Cloud formation in the atomic and molecular phase |b H I self absorption (HISA) towards a giant molecular filament |c Y. Wang, S. Bihr, H. Beuther, M.R. Rugel, J.D. Soler, J. Ott, J. Kainulainen, N. Schneider, R.S. Klessen, S.C.O. Glover, N.M. McClure-Griffiths, P.F. Goldsmith, K.G. Johnston, K.M. Menten, S. Ragan, L.D. Anderson, J.S. Urquhart, H. Linz, N. Roy, R.J. Smith, F. Bigiel, T. Henning, and S.N. Longmore |
| 264 | 1 | |c February 2020 | |
| 300 | |a 21 | ||
| 336 | |a Text |b txt |2 rdacontent | ||
| 337 | |a Computermedien |b c |2 rdamedia | ||
| 338 | |a Online-Ressource |b cr |2 rdacarrier | ||
| 500 | |a Gesehen am 25.01.2021 | ||
| 520 | |a Molecular clouds form from the atomic phase of the interstellar medium. However, characterizing the transition between the atomic and the molecular interstellar medium (ISM) is a complex observational task. Here we address cloud formation processes by combining H I self absorption (HISA) with molecular line data. Column density probability density functions (N-PDFs) are a common tool for examining molecular clouds. One scenario proposed by numerical simulations is that the N-PDF evolves from a log-normal shape at early times to a power-law-like shape at later times. To date, investigations of N-PDFs have been mostly limited to the molecular component of the cloud. In this paper, we study the cold atomic component of the giant molecular filament GMF38.1-32.4a (GMF38a, distance = 3.4 kpc, length ~ 230 pc), calculate its N-PDFs, and study its kinematics. We identify an extended HISA feature, which is partly correlated with the <sup>13<sup/>CO emission. The peak velocities of the HISA and <sup>13<sup/>CO observations agree well on the eastern side of the filament, whereas a velocity offset of approximately 4 km s<sup>−1<sup/> is found on the western side. The sonic Mach number we derive from the linewidth measurements shows that a large fraction of the HISA, which is ascribed to the cold neutral medium (CNM), is at subsonic and transonic velocities. The column density of the CNM part is on the order of 10<sup>20<sup/> to 10<sup>21<sup/> cm<sup>−2<sup/>. The column density of molecular hydrogen, traced by <sup>13<sup/>CO, is an order of magnitude higher. The N-PDFs from HISA (CNM), H I emission (the warm and cold neutral medium), and <sup>13<sup/>CO (molecular component) are well described by log-normal functions, which is in agreement with turbulent motions being the main driver of cloud dynamics. The N-PDF of the molecular component also shows a power law in the high column-density region, indicating self-gravity. We suggest that we are witnessing two different evolutionary stages within the filament. The eastern subregion seems to be forming a molecular cloud out of the atomic gas, whereas the western subregion already shows high column density peaks, active star formation, and evidence of related feedback processes. | ||
| 700 | 1 | |a Bihr, Simon |e VerfasserIn |0 (DE-588)1100902783 |0 (DE-627)859623041 |0 (DE-576)469827629 |4 aut | |
| 700 | 1 | |a Beuther, Henrik |d 1971- |e VerfasserIn |0 (DE-588)1181461847 |0 (DE-627)1662669143 |4 aut | |
| 700 | 1 | |a Rugel, Michael |d 1990- |e VerfasserIn |0 (DE-588)1173911278 |0 (DE-627)1043713239 |0 (DE-576)515785032 |4 aut | |
| 700 | 1 | |a Soler, Juan D. |e VerfasserIn |0 (DE-588)1156954401 |0 (DE-627)1019898232 |0 (DE-576)502354801 |4 aut | |
| 700 | 1 | |a Ott, J. |e VerfasserIn |4 aut | |
| 700 | 1 | |a Kainulainen, J. |e VerfasserIn |4 aut | |
| 700 | 1 | |a Schneider, N. |e VerfasserIn |4 aut | |
| 700 | 1 | |a Klessen, Ralf S. |d 1968- |e VerfasserIn |0 (DE-588)120533820 |0 (DE-627)392381532 |0 (DE-576)178685399 |4 aut | |
| 700 | 1 | |a Glover, S. C. O. |e VerfasserIn |4 aut | |
| 700 | 1 | |a McClure-Griffiths, N. M. |e VerfasserIn |4 aut | |
| 700 | 1 | |a Goldsmith, P. F. |e VerfasserIn |4 aut | |
| 700 | 1 | |a Johnston, K. G. |e VerfasserIn |4 aut | |
| 700 | 1 | |a Menten, K. M. |e VerfasserIn |4 aut | |
| 700 | 1 | |a Ragan, S. |e VerfasserIn |4 aut | |
| 700 | 1 | |a Anderson, L. D. |e VerfasserIn |4 aut | |
| 700 | 1 | |a Urquhart, J. S. |e VerfasserIn |4 aut | |
| 700 | 1 | |a Linz, Hendrik |d 1975- |e VerfasserIn |0 (DE-588)130330140 |0 (DE-627)707463718 |0 (DE-576)250684985 |4 aut | |
| 700 | 1 | |a Roy, N. |e VerfasserIn |4 aut | |
| 700 | 1 | |a Smith, R. J. |e VerfasserIn |4 aut | |
| 700 | 1 | |a Bigiel, F. |e VerfasserIn |4 aut | |
| 700 | 1 | |a Henning, Thomas |d 1956- |e VerfasserIn |0 (DE-588)124568637 |0 (DE-627)526967811 |0 (DE-576)294236120 |4 aut | |
| 700 | 1 | |a Longmore, S. N. |e VerfasserIn |4 aut | |
| 773 | 0 | 8 | |i Enthalten in |t Astronomy and astrophysics |d Les Ulis : EDP Sciences, 1969 |g 634(2020) Artikel-Nummer A139, 21 Seiten |h Online-Ressource |w (DE-627)253390222 |w (DE-600)1458466-9 |w (DE-576)072283351 |x 1432-0746 |7 nnas |a Cloud formation in the atomic and molecular phase H I self absorption (HISA) towards a giant molecular filament |
| 773 | 1 | 8 | |g volume:634 |g year:2020 |g extent:21 |a Cloud formation in the atomic and molecular phase H I self absorption (HISA) towards a giant molecular filament |
| 856 | 4 | 0 | |u https://dx.doi.org/10.1051/0004-6361/201935866 |x Verlag |x Resolving-System |z lizenzpflichtig |3 Volltext |
| 856 | 4 | 0 | |u https://www.aanda.org/articles/aa/abs/2020/02/aa35866-19/aa35866-19.html |x Verlag |z lizenzpflichtig |3 Volltext |
| 951 | |a AR | ||
| 992 | |a 20210125 | ||
| 993 | |a Article | ||
| 994 | |a 2020 | ||
| 998 | |g 124568637 |a Henning, Thomas |m 124568637:Henning, Thomas |d 130000 |d 700000 |d 728500 |e 130000PH124568637 |e 700000PH124568637 |e 728500PH124568637 |k 0/130000/ |k 0/700000/ |k 1/700000/728500/ |p 22 | ||
| 998 | |g 130330140 |a Linz, Hendrik |m 130330140:Linz, Hendrik |p 18 | ||
| 998 | |g 120533820 |a Klessen, Ralf S. |m 120533820:Klessen, Ralf S. |d 700000 |d 714000 |d 714200 |d 700000 |d 728500 |e 700000PK120533820 |e 714000PK120533820 |e 714200PK120533820 |e 700000PK120533820 |e 728500PK120533820 |k 0/700000/ |k 1/700000/714000/ |k 2/700000/714000/714200/ |k 0/700000/ |k 1/700000/728500/ |p 9 | ||
| 998 | |g 1173911278 |a Rugel, Michael |m 1173911278:Rugel, Michael |p 4 | ||
| 998 | |g 1181461847 |a Beuther, Henrik |m 1181461847:Beuther, Henrik |d 130000 |e 130000PB1181461847 |k 0/130000/ |p 3 | ||
| 998 | |g 1100902783 |a Bihr, Simon |m 1100902783:Bihr, Simon |d 700000 |d 714000 |d 714200 |e 700000PB1100902783 |e 714000PB1100902783 |e 714200PB1100902783 |k 0/700000/ |k 1/700000/714000/ |k 2/700000/714000/714200/ |p 2 | ||
| 999 | |a KXP-PPN1745593896 |e 3842297904 | ||
| BIB | |a Y | ||
| SER | |a journal | ||
| JSO | |a {"relHost":[{"note":["Gesehen am 21.06.2024","Erscheint 36mal jährlich in 12 Bänden zu je 3 Ausgaben","Fortsetzung der Druck-Ausgabe"],"type":{"bibl":"periodical","media":"Online-Ressource"},"origin":[{"dateIssuedKey":"1969","dateIssuedDisp":"1969-","publisherPlace":"Les Ulis ; Berlin ; Heidelberg","publisher":"EDP Sciences ; Springer"}],"title":[{"title":"Astronomy and astrophysics","title_sort":"Astronomy and astrophysics","subtitle":"an international weekly journal"}],"pubHistory":["1.1969 -"],"language":["eng"],"titleAlt":[{"title":"Astronomy & astrophysics"},{"title":"a European journal"}],"physDesc":[{"extent":"Online-Ressource"}],"disp":"Cloud formation in the atomic and molecular phase H I self absorption (HISA) towards a giant molecular filamentAstronomy and astrophysics","corporate":[{"display":"European Southern Observatory","role":"isb"}],"part":{"text":"634(2020) Artikel-Nummer A139, 21 Seiten","year":"2020","extent":"21","volume":"634"},"name":{"displayForm":["European Southern Observatory (ESO)"]},"id":{"eki":["253390222"],"zdb":["1458466-9"],"issn":["1432-0746"]},"recId":"253390222"}],"name":{"displayForm":["Y. Wang, S. Bihr, H. Beuther, M.R. Rugel, J.D. Soler, J. Ott, J. Kainulainen, N. Schneider, R.S. Klessen, S.C.O. Glover, N.M. McClure-Griffiths, P.F. Goldsmith, K.G. Johnston, K.M. Menten, S. Ragan, L.D. Anderson, J.S. Urquhart, H. Linz, N. Roy, R.J. Smith, F. Bigiel, T. Henning, and S.N. Longmore"]},"id":{"doi":["10.1051/0004-6361/201935866"],"eki":["1745593896"]},"recId":"1745593896","language":["eng"],"physDesc":[{"extent":"21 S."}],"type":{"media":"Online-Ressource","bibl":"article-journal"},"origin":[{"dateIssuedDisp":"February 2020","dateIssuedKey":"2020"}],"title":[{"title":"Cloud formation in the atomic and molecular phase","title_sort":"Cloud formation in the atomic and molecular phase","subtitle":"H I self absorption (HISA) towards a giant molecular filament"}],"person":[{"role":"aut","family":"Wang","given":"Yuan","display":"Wang, Yuan"},{"role":"aut","display":"Bihr, Simon","given":"Simon","family":"Bihr"},{"role":"aut","family":"Beuther","given":"Henrik","display":"Beuther, Henrik"},{"role":"aut","given":"Michael","family":"Rugel","display":"Rugel, Michael"},{"role":"aut","given":"Juan D.","family":"Soler","display":"Soler, Juan D."},{"family":"Ott","given":"J.","display":"Ott, J.","role":"aut"},{"given":"J.","family":"Kainulainen","display":"Kainulainen, J.","role":"aut"},{"family":"Schneider","given":"N.","display":"Schneider, N.","role":"aut"},{"role":"aut","given":"Ralf S.","family":"Klessen","display":"Klessen, Ralf S."},{"family":"Glover","given":"S. C. O.","display":"Glover, S. C. O.","role":"aut"},{"role":"aut","display":"McClure-Griffiths, N. M.","given":"N. M.","family":"McClure-Griffiths"},{"display":"Goldsmith, P. F.","given":"P. F.","family":"Goldsmith","role":"aut"},{"family":"Johnston","given":"K. G.","display":"Johnston, K. G.","role":"aut"},{"display":"Menten, K. M.","family":"Menten","given":"K. M.","role":"aut"},{"role":"aut","display":"Ragan, S.","given":"S.","family":"Ragan"},{"role":"aut","family":"Anderson","given":"L. D.","display":"Anderson, L. D."},{"given":"J. S.","family":"Urquhart","display":"Urquhart, J. S.","role":"aut"},{"role":"aut","given":"Hendrik","family":"Linz","display":"Linz, Hendrik"},{"family":"Roy","given":"N.","display":"Roy, N.","role":"aut"},{"display":"Smith, R. J.","family":"Smith","given":"R. J.","role":"aut"},{"given":"F.","family":"Bigiel","display":"Bigiel, F.","role":"aut"},{"family":"Henning","given":"Thomas","display":"Henning, Thomas","role":"aut"},{"role":"aut","family":"Longmore","given":"S. N.","display":"Longmore, S. N."}],"note":["Gesehen am 25.01.2021"]} | ||
| SRT | |a WANGYUANBICLOUDFORMA2020 | ||