Temperature Structures of Embedded Disks: Young Disks in Taurus Are Warm

Research output: Contribution to journal › Journal article › Research › peer-review

Standard

Temperature Structures of Embedded Disks : Young Disks in Taurus Are Warm. / Hoff, Merel L. R. van 't; Harsono, Daniel; Tobin, John J.; Bosman, Arthur D.; van Dishoeck, Ewine F.; Jorgensen, Jes K.; Miotello, Anna; Murillo, Nadia M.; Walsh, Catherine.

In: Astrophysical Journal, Vol. 901, No. 2, 166, 10.2020.

Research output: Contribution to journal › Journal article › Research › peer-review

Harvard

Hoff, MLRV, Harsono, D, Tobin, JJ, Bosman, AD, van Dishoeck, EF, Jorgensen, JK, Miotello, A, Murillo, NM & Walsh, C 2020, 'Temperature Structures of Embedded Disks: Young Disks in Taurus Are Warm', Astrophysical Journal, vol. 901, no. 2, 166. https://doi.org/10.3847/1538-4357/abb1a2

APA

Hoff, M. L. R. V. ., Harsono, D., Tobin, J. J., Bosman, A. D., van Dishoeck, E. F., Jorgensen, J. K., Miotello, A., Murillo, N. M., & Walsh, C. (2020). Temperature Structures of Embedded Disks: Young Disks in Taurus Are Warm. Astrophysical Journal, 901(2), [166]. https://doi.org/10.3847/1538-4357/abb1a2

Vancouver

Hoff MLRV, Harsono D, Tobin JJ, Bosman AD, van Dishoeck EF, Jorgensen JK et al. Temperature Structures of Embedded Disks: Young Disks in Taurus Are Warm. Astrophysical Journal. 2020 Oct;901(2). 166. https://doi.org/10.3847/1538-4357/abb1a2

Author

Hoff, Merel L. R. van 't ; Harsono, Daniel ; Tobin, John J. ; Bosman, Arthur D. ; van Dishoeck, Ewine F. ; Jorgensen, Jes K. ; Miotello, Anna ; Murillo, Nadia M. ; Walsh, Catherine. / Temperature Structures of Embedded Disks : Young Disks in Taurus Are Warm. In: Astrophysical Journal. 2020 ; Vol. 901, No. 2.

Bibtex

@article{bb988db625944df1890db5cc21eefdf2,
title = "Temperature Structures of Embedded Disks: Young Disks in Taurus Are Warm",
abstract = "The chemical composition of gas and ice in disks around young stars sets the bulk composition of planets. In contrast to protoplanetary disks (Class II), young disks that are still embedded in their natal envelope (Class 0 and I) are predicted to be too warm for CO to freeze out, as has been confirmed observationally for L1527 IRS. To establish whether young disks are generally warmer than their more evolved counterparts, we observed five young (Class 0/I and I) disks in Taurus with the Atacama Large Millimeter/submillimeter Array, targeting (CO)-O-17 2 - 1, H2CO",
keywords = "Protostars, Protoplanetary disks, Young stellar objects, Astrochemistry, LOW-MASS PROTOSTARS, PROTOPLANETARY DISKS, T-TAURI, CIRCUMSTELLAR DISKS, PLANET FORMATION, MOLECULAR CLOUD, ALMA SURVEY, SUBMILLIMETER, ACCRETION, CO",
author = "Hoff, {Merel L. R. van 't} and Daniel Harsono and Tobin, {John J.} and Bosman, {Arthur D.} and {van Dishoeck}, {Ewine F.} and Jorgensen, {Jes K.} and Anna Miotello and Murillo, {Nadia M.} and Catherine Walsh",
year = "2020",
month = oct,
doi = "10.3847/1538-4357/abb1a2",
language = "English",
volume = "901",
journal = "Astrophysical Journal",
issn = "0004-637X",
publisher = "Institute of Physics Publishing, Inc",
number = "2",

}

RIS

TY - JOUR

T1 - Temperature Structures of Embedded Disks

T2 - Young Disks in Taurus Are Warm

AU - Hoff, Merel L. R. van 't

AU - Harsono, Daniel

AU - Tobin, John J.

AU - Bosman, Arthur D.

AU - van Dishoeck, Ewine F.

AU - Jorgensen, Jes K.

AU - Miotello, Anna

AU - Murillo, Nadia M.

AU - Walsh, Catherine

PY - 2020/10

Y1 - 2020/10

N2 - The chemical composition of gas and ice in disks around young stars sets the bulk composition of planets. In contrast to protoplanetary disks (Class II), young disks that are still embedded in their natal envelope (Class 0 and I) are predicted to be too warm for CO to freeze out, as has been confirmed observationally for L1527 IRS. To establish whether young disks are generally warmer than their more evolved counterparts, we observed five young (Class 0/I and I) disks in Taurus with the Atacama Large Millimeter/submillimeter Array, targeting (CO)-O-17 2 - 1, H2CO

AB - The chemical composition of gas and ice in disks around young stars sets the bulk composition of planets. In contrast to protoplanetary disks (Class II), young disks that are still embedded in their natal envelope (Class 0 and I) are predicted to be too warm for CO to freeze out, as has been confirmed observationally for L1527 IRS. To establish whether young disks are generally warmer than their more evolved counterparts, we observed five young (Class 0/I and I) disks in Taurus with the Atacama Large Millimeter/submillimeter Array, targeting (CO)-O-17 2 - 1, H2CO

KW - Protostars

KW - Protoplanetary disks

KW - Young stellar objects

KW - Astrochemistry

KW - LOW-MASS PROTOSTARS

KW - PROTOPLANETARY DISKS

KW - T-TAURI

KW - CIRCUMSTELLAR DISKS

KW - PLANET FORMATION

KW - MOLECULAR CLOUD

KW - ALMA SURVEY

KW - SUBMILLIMETER

KW - ACCRETION

KW - CO

U2 - 10.3847/1538-4357/abb1a2

DO - 10.3847/1538-4357/abb1a2

M3 - Journal article

VL - 901

JO - Astrophysical Journal

JF - Astrophysical Journal

SN - 0004-637X

IS - 2

M1 - 166

ER -

ID: 250553135