Show/Hide Menu
Hide/Show Apps
Logout
Türkçe
Türkçe
Search
Search
Login
Login
OpenMETU
OpenMETU
About
About
Open Science Policy
Open Science Policy
Open Access Guideline
Open Access Guideline
Postgraduate Thesis Guideline
Postgraduate Thesis Guideline
Communities & Collections
Communities & Collections
Help
Help
Frequently Asked Questions
Frequently Asked Questions
Guides
Guides
Thesis submission
Thesis submission
MS without thesis term project submission
MS without thesis term project submission
Publication submission with DOI
Publication submission with DOI
Publication submission
Publication submission
Supporting Information
Supporting Information
General Information
General Information
Copyright, Embargo and License
Copyright, Embargo and License
Contact us
Contact us
Dust, Ice, and Gas In Time (DIGIT) <i>Herschel</i> program first results A full PACS-SED scan of the gas line emission in protostar DK Chamaeleontis
Date
2010-07-01
Author
van Kempen, T. A.
Green, J. D.
Evans, N. J.
van Dishoeck, E. F.
Kristensen, L. E.
Herczeg, G. J.
Merin, B.
Lee, J. -E.
Jorgensen, J. K.
Bouwman, J.
Acke, B.
Adamkovics, M.
Augereau, J. C.
Bergin, E.
Blake, G. A.
Brown, J. M.
Carr, J. S.
Chen, J. -H.
Cieza, L.
Dominik, C.
Dullemond, C. P.
Dunham, M. M.
Glassgold, A.
Guedel, M.
Harvey, P. M.
Henning, Th.
Hogerheijde, M. R.
Jaffe, D.
Kim, H. J.
Knez, C.
Lacy, J. H.
Maret, S.
Meeus, G.
Meijerink, R.
Mulders, G. D.
Mundy, L.
Najita, J.
Olofsson, J.
Pontoppidan, K. M.
Salyk, C.
Sturm, B.
Visser, R.
Waters, L. B. F. M.
Waelkens, C.
Yıldız, Umut
Metadata
Show full item record
This work is licensed under a
Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License
.
Item Usage Stats
9
views
0
downloads
Cite This
Aims. We aim to study the composition and energetics of the circumstellar material of DK Cha, an intermediate-mass star in transition from an embedded configuration to a star plus disk stage, during this pivotal stage of its evolution. Methods. Using the range scan mode of PACS on the Herschel Space Observatory, we obtained a spectrum of DK Cha from 55 to 210 mu m as part of the DIGIT key program. Results. Almost 50 molecular and atomic lines were detected, many more than the 7 lines detected in ISO-LWS. Nearly the entire ladder of CO from J = 14-13 to 38-37 (E-u/k = 4080 K), water from levels as excited as J(K-1K+1) = 7(07) (E-u/k = 843 K), and OH lines up to E-u/k = 290 K were detected. Conclusions. The continuum emission in our PACS SED scan matches the flux expected by a model consisting of a star, a surrounding disk of 0.03 M-circle dot, and an envelope of a similar mass, supporting the suggestion that the object is emerging from its main accretion stage. Molecular, atomic, and ionic emission lines in the far-infrared reveal the outflow's influence on the envelope. The inferred hot gas may be photon-heated, but some emission may be caused by C-shocks in the walls of the outflow cavity.
URI
https://hdl.handle.net/11511/115891
Journal
ASTRONOMY & ASTROPHYSICS
DOI
https://doi.org/10.1051/0004-6361/201014686
Collections
Department of Physics, Article
Citation Formats
IEEE
ACM
APA
CHICAGO
MLA
BibTeX
T. A. van Kempen et al., “Dust, Ice, and Gas In Time (DIGIT) <i>Herschel</i> program first results A full PACS-SED scan of the gas line emission in protostar DK Chamaeleontis,”
ASTRONOMY & ASTROPHYSICS
, vol. 518, pp. 0–0, 2010, Accessed: 00, 2025. [Online]. Available: https://hdl.handle.net/11511/115891.