The fragmentation criteria in local vertically stratified self-gravitating disk simulations
Massive circumstellar disks are prone to gravitational instabilities, which trigger the formation of spiral arms that can fragment into bound clumps under the right conditions. Two-dimensional simulations of self-gravitating disks are useful starting points for studying fragmentation because they al...
Gespeichert in:
| Hauptverfasser: | , , |
|---|---|
| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
2017 October 9
|
| In: |
The astrophysical journal
Year: 2017, Jahrgang: 848, Heft: 1, Pages: 40 |
| ISSN: | 1538-4357 |
| DOI: | 10.3847/1538-4357/aa8a66 |
| Online-Zugang: | Verlag, kostenfrei, Volltext: https://doi.org/10.3847/1538-4357/aa8a66 Verlag: https://doi.org/10.3847%2F1538-4357%2Faa8a66 
|
| Verfasserangaben: | Hans Baehr, Hubert Klahr, and Kaitlin M. Kratter |
MARC
| LEADER | 00000caa a2200000 c 4500 | ||
|---|---|---|---|
| 001 | 1725614847 | ||
| 003 | DE-627 | ||
| 005 | 20220818161935.0 | ||
| 007 | cr uuu---uuuuu | ||
| 008 | 200727s2017 xx |||||o 00| ||eng c | ||
| 024 | 7 | |a 10.3847/1538-4357/aa8a66 |2 doi | |
| 035 | |a (DE-627)1725614847 | ||
| 035 | |a (DE-599)KXP1725614847 | ||
| 035 | |a (OCoLC)1341347923 | ||
| 040 | |a DE-627 |b ger |c DE-627 |e rda | ||
| 041 | |a eng | ||
| 084 | |a 29 |2 sdnb | ||
| 100 | 1 | |a Baehr, Hans-Paul Frederick |d 1989- |e VerfasserIn |0 (DE-588)1193198461 |0 (DE-627)1671846834 |4 aut | |
| 245 | 1 | 4 | |a The fragmentation criteria in local vertically stratified self-gravitating disk simulations |c Hans Baehr, Hubert Klahr, and Kaitlin M. Kratter |
| 264 | 1 | |c 2017 October 9 | |
| 300 | |a 10 | ||
| 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 27.07.2020 | ||
| 520 | |a Massive circumstellar disks are prone to gravitational instabilities, which trigger the formation of spiral arms that can fragment into bound clumps under the right conditions. Two-dimensional simulations of self-gravitating disks are useful starting points for studying fragmentation because they allow high-resolution simulations of thin disks. However, convergence issues can arise in 2D from various sources. One of these sources is the 2D approximation of self-gravity, which exaggerates the effect of self-gravity on small scales when the potential is not smoothed to account for the assumed vertical extent of the disk. This effect is enhanced by increased resolution, resulting in fragmentation at longer cooling timescales β. If true, it suggests that the 3D simulations of disk fragmentation may not have the same convergence problem and could be used to examine the nature of fragmentation without smoothing self-gravity on scales similar to the disk scale height. To that end, we have carried out local 3D self-gravitating disk simulations with simple β cooling with fixed background irradiation to determine if 3D is necessary to properly describe disk fragmentation. Above a resolution of ∼40 grid cells per scale height, we find that our simulations converge with respect to the cooling timescale. This result converges in agreement with analytic expectations which place a fragmentation boundary at β crit = 3. | ||
| 700 | 1 | |a Klahr, Hubert |d 1966- |e VerfasserIn |0 (DE-588)1098340302 |0 (DE-627)857553844 |0 (DE-576)469081724 |4 aut | |
| 700 | 1 | |a Kratter, Kaitlin |e VerfasserIn |0 (DE-588)1214759483 |0 (DE-627)1725856794 |4 aut | |
| 773 | 0 | 8 | |i Enthalten in |t The astrophysical journal |d London : Institute of Physics Publ., 1995 |g 848(2017,1) Artikel-Nummer 40, 10 Seiten |h Online-Ressource |w (DE-627)269019219 |w (DE-600)1473835-1 |w (DE-576)077662733 |x 1538-4357 |7 nnas |a The fragmentation criteria in local vertically stratified self-gravitating disk simulations |
| 773 | 1 | 8 | |g volume:848 |g year:2017 |g number:1 |g pages:40 |g extent:10 |a The fragmentation criteria in local vertically stratified self-gravitating disk simulations |
| 856 | 4 | 0 | |u https://doi.org/10.3847/1538-4357/aa8a66 |x Verlag |x Resolving-System |z kostenfrei |3 Volltext |
| 856 | 4 | 0 | |u https://doi.org/10.3847%2F1538-4357%2Faa8a66 |x Verlag |
| 951 | |a AR | ||
| 992 | |a 20200727 | ||
| 993 | |a Article | ||
| 994 | |a 2017 | ||
| 998 | |g 1098340302 |a Klahr, Hubertus |m 1098340302:Klahr, Hubertus |d 130000 |e 130000PK1098340302 |k 0/130000/ |p 2 | ||
| 999 | |a KXP-PPN1725614847 |e 3729546104 | ||
| BIB | |a Y | ||
| SER | |a journal | ||
| JSO | |a {"title":[{"title_sort":"fragmentation criteria in local vertically stratified self-gravitating disk simulations","title":"The fragmentation criteria in local vertically stratified self-gravitating disk simulations"}],"person":[{"family":"Baehr","given":"Hans-Paul Frederick","roleDisplay":"VerfasserIn","display":"Baehr, Hans-Paul Frederick","role":"aut"},{"given":"Hubert","family":"Klahr","role":"aut","display":"Klahr, Hubert","roleDisplay":"VerfasserIn"},{"family":"Kratter","given":"Kaitlin","display":"Kratter, Kaitlin","roleDisplay":"VerfasserIn","role":"aut"}],"note":["Gesehen am 27.07.2020"],"type":{"bibl":"article-journal","media":"Online-Ressource"},"recId":"1725614847","language":["eng"],"origin":[{"dateIssuedKey":"2017","dateIssuedDisp":"2017 October 9"}],"id":{"doi":["10.3847/1538-4357/aa8a66"],"eki":["1725614847"]},"name":{"displayForm":["Hans Baehr, Hubert Klahr, and Kaitlin M. Kratter"]},"physDesc":[{"extent":"10 S."}],"relHost":[{"title":[{"title":"The astrophysical journal","subtitle":"an international review of spectroscopy and astronomical physics","title_sort":"astrophysical journal"}],"pubHistory":["Vol. 447 (1995) [?]-"],"titleAlt":[{"title":"The astrophysical journal / 1"},{"title":"ApJ"}],"part":{"year":"2017","pages":"40","issue":"1","volume":"848","text":"848(2017,1) Artikel-Nummer 40, 10 Seiten","extent":"10"},"disp":"The fragmentation criteria in local vertically stratified self-gravitating disk simulationsThe astrophysical journal","note":["Gesehen am 18.01.2022","Fortsetzung der Druck-Ausgabe"],"type":{"bibl":"periodical","media":"Online-Ressource"},"recId":"269019219","language":["eng"],"origin":[{"publisherPlace":"London ; Chicago, Ill. [u.a.]","dateIssuedDisp":"[1995?]-","publisher":"Institute of Physics Publ. ; Univ. of Chicago Press"}],"id":{"issn":["1538-4357"],"eki":["269019219"],"zdb":["1473835-1"]},"name":{"displayForm":["publ. in coll. with the American Astronomical Society. S. Chandrasekhar, managing ed"]},"physDesc":[{"extent":"Online-Ressource"}]}]} | ||
| SRT | |a BAEHRHANSPFRAGMENTAT2017 | ||