Growth of grains in brown dwarf disks
We perform coagulation and fragmentation simulations using the new physically motivated model by Garaud et al. to determine growth locally in brown dwarf disks. We show that large grains can grow and that if brown dwarf disks are scaled-down versions of T Tauri disks (in terms of stellar mass, disk...
Gespeichert in:
| Hauptverfasser: | , , |
|---|---|
| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
2013 August 12
|
| In: |
The astrophysical journal. Part 2, Letters
Year: 2013, Jahrgang: 774, Heft: 1, Pages: 1-5 |
| ISSN: | 2041-8213 |
| DOI: | 10.1088/2041-8205/774/1/L4 |
| Online-Zugang: | Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1088/2041-8205/774/1/L4
|
| Verfasserangaben: | Farzana Meru, Marina Galvagni, and Christoph Olczak |
MARC
| LEADER | 00000caa a2200000 c 4500 | ||
|---|---|---|---|
| 001 | 1758243732 | ||
| 003 | DE-627 | ||
| 005 | 20220819212518.0 | ||
| 007 | cr uuu---uuuuu | ||
| 008 | 210520s2013 xx |||||o 00| ||eng c | ||
| 024 | 7 | |a 10.1088/2041-8205/774/1/L4 |2 doi | |
| 035 | |a (DE-627)1758243732 | ||
| 035 | |a (DE-599)KXP1758243732 | ||
| 035 | |a (OCoLC)1341413727 | ||
| 040 | |a DE-627 |b ger |c DE-627 |e rda | ||
| 041 | |a eng | ||
| 084 | |a 29 |2 sdnb | ||
| 100 | 1 | |a Meru, Farzana |e VerfasserIn |0 (DE-588)1233996991 |0 (DE-627)175843936X |4 aut | |
| 245 | 1 | 0 | |a Growth of grains in brown dwarf disks |c Farzana Meru, Marina Galvagni, and Christoph Olczak |
| 264 | 1 | |c 2013 August 12 | |
| 300 | |a 5 | ||
| 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 20.05.2021 | ||
| 520 | |a We perform coagulation and fragmentation simulations using the new physically motivated model by Garaud et al. to determine growth locally in brown dwarf disks. We show that large grains can grow and that if brown dwarf disks are scaled-down versions of T Tauri disks (in terms of stellar mass, disk mass, and disk radius) growth at an equivalent location with respect to the disk truncation radius can occur to the same size in both disks. We show that similar growth occurs because the collisional timescales in the two disks are comparable. Our model may therefore potentially explain the recent observations of grain growth to millimeter sizes in brown dwarf disks, as seen in T Tauri disks. | ||
| 700 | 1 | |a Galvagni, Marina |e VerfasserIn |0 (DE-588)1235001725 |0 (DE-627)1760017922 |4 aut | |
| 700 | 1 | |a Olczak, Christoph |e VerfasserIn |0 (DE-588)1042644918 |0 (DE-627)76916451X |0 (DE-576)31455114X |4 aut | |
| 773 | 0 | 8 | |i Enthalten in |t The astrophysical journal. Part 2, Letters |d London : Institute of Physics Publ., 1995 |g 774(2013), 1, Artikel-ID L4, Seite 1-5 |h Online-Ressource |w (DE-627)312189028 |w (DE-600)2006858-X |w (DE-576)090890876 |x 2041-8213 |7 nnas |a Growth of grains in brown dwarf disks |
| 773 | 1 | 8 | |g volume:774 |g year:2013 |g number:1 |g elocationid:L4 |g pages:1-5 |g extent:5 |a Growth of grains in brown dwarf disks |
| 856 | 4 | 0 | |u https://doi.org/10.1088/2041-8205/774/1/L4 |x Verlag |x Resolving-System |z lizenzpflichtig |3 Volltext |
| 951 | |a AR | ||
| 992 | |a 20210520 | ||
| 993 | |a Article | ||
| 994 | |a 2013 | ||
| 998 | |g 1042644918 |a Olczak, Christoph |m 1042644918:Olczak, Christoph |d 700000 |d 714000 |d 714100 |e 700000PO1042644918 |e 714000PO1042644918 |e 714100PO1042644918 |k 0/700000/ |k 1/700000/714000/ |k 2/700000/714000/714100/ |p 3 |y j | ||
| 999 | |a KXP-PPN1758243732 |e 3929864096 | ||
| BIB | |a Y | ||
| SER | |a journal | ||
| JSO | |a {"person":[{"family":"Meru","given":"Farzana","roleDisplay":"VerfasserIn","display":"Meru, Farzana","role":"aut"},{"given":"Marina","family":"Galvagni","role":"aut","roleDisplay":"VerfasserIn","display":"Galvagni, Marina"},{"display":"Olczak, Christoph","roleDisplay":"VerfasserIn","role":"aut","family":"Olczak","given":"Christoph"}],"title":[{"title":"Growth of grains in brown dwarf disks","title_sort":"Growth of grains in brown dwarf disks"}],"recId":"1758243732","language":["eng"],"note":["Gesehen am 20.05.2021"],"type":{"bibl":"article-journal","media":"Online-Ressource"},"name":{"displayForm":["Farzana Meru, Marina Galvagni, and Christoph Olczak"]},"id":{"eki":["1758243732"],"doi":["10.1088/2041-8205/774/1/L4"]},"origin":[{"dateIssuedKey":"2013","dateIssuedDisp":"2013 August 12"}],"relHost":[{"origin":[{"dateIssuedDisp":"1995-","dateIssuedKey":"1995","publisher":"Institute of Physics Publ. ; Univ. of Chicago Press","publisherPlace":"London ; Chicago, Ill. [u.a.]"}],"id":{"issn":["2041-8213"],"zdb":["2006858-X"],"eki":["312189028"]},"physDesc":[{"extent":"Online-Ressource"}],"title":[{"partname":"Letters","title":"The astrophysical journal","title_sort":"astrophysical journal"}],"pubHistory":["Nachgewiesen 447.1995 -"],"part":{"pages":"1-5","issue":"1","year":"2013","extent":"5","text":"774(2013), 1, Artikel-ID L4, Seite 1-5","volume":"774"},"titleAlt":[{"title":"The astrophysical journal / 2"},{"title":"ApJL"}],"disp":"Growth of grains in brown dwarf disksThe astrophysical journal. Part 2, Letters","note":["Fortsetzung der Druck-Ausgabe","Frühere Jahrgänge online nicht mehr verfügbar","Gesehen am 18.01.2022"],"type":{"media":"Online-Ressource","bibl":"periodical"},"recId":"312189028","language":["eng"]}],"physDesc":[{"extent":"5 S."}]} | ||
| SRT | |a MERUFARZANGROWTHOFGR2013 | ||