Zobrazeno 1 - 8
of 8
pro vyhledávání: '"David Madlener"'
Publikováno v:
Acta Polytechnica CTU Proceedings, Vol 38, Pp 613–619-613–619 (2022)
The question of future energy-efficient creation of living space is becoming more and more important in many cities due to limited space availability and simultaneously increasing settlement pressure. Against the background of the desired space, reso
Externí odkaz:
https://doaj.org/article/996ec9975acc4130845a282ef48dc843
Publikováno v:
Research in Astronomy and Astrophysics. 13:841-848
We present modeling work on three young stellar objects that are promising targets for future high-resolution observations to investigate circumstellar disk evolution. The currently available data comprise the spectral energy distribution from optica
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d96886515986db1e0236f9d2714a3e1b
https://doi.org/10.1088/1674-4527/13/7/008
https://doi.org/10.1088/1674-4527/13/7/008
Publikováno v:
Research in Astronomy and Astrophysics. 13:420-434
We present a detailed comparison of two approaches, the use of a pre-calculated database and simulated annealing (SA), for fitting the continuum spectral energy distribution (SED) of astrophysical objects whose appearance is dominated by surrounding
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6b4e1194ba391ff74988f98b8ec2f4b6
https://doi.org/10.1088/1674-4527/13/4/005
https://doi.org/10.1088/1674-4527/13/4/005
Protoplanetary disks are a byproduct of the star formation process. In the dense mid-plane of these disks, planetesimals and planets are expected to form. The first step in planet formation is the growth of dust particles from submicrometer-sized gra
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4d14526db871ce6f932c5fc6653e609e
http://arxiv.org/abs/1607.05449
http://arxiv.org/abs/1607.05449
Autor:
Hans-Herbert Fischer, Istvan Apathy, Attila Peter, Michael Kretschmer, David Madlener, Sascha Schieke, Walter Arnold, Klaus J. Seidensticker, K. Thiel, D. Möhlmann, Walter Schmidt, Roland Trautner
Publikováno v:
Space Science Reviews. 128:301-337
SESAME is an instrument complex built in international co-operation and carried by the Rosetta lander Philae intended to land on comet 67P/Churyumov-Gerasimenko in 2014. The main goals of this instrument suite are to measure mechanical and electrical
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9333d6c181521cb986fc251f6d08afbc
https://doi.org/10.1007/s11214-006-9118-6
https://doi.org/10.1007/s11214-006-9118-6
Publikováno v:
Astronomy and Geophysics
Astronomy and Geophysics, Oxford University Press (OUP), 2012, 543, pp.A81. ⟨10.1051/0004-6361/201117615⟩
EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France, p.409, 2011
EPSC-DPS Joint Meeting 2011
EPSC-DPS Joint Meeting 2011, 2011, Nantes, France. pp.409
Astronomy and Geophysics, Oxford University Press (OUP), 2012, 543, pp.A81. ⟨10.1051/0004-6361/201117615⟩
EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France, p.409, 2011
EPSC-DPS Joint Meeting 2011
EPSC-DPS Joint Meeting 2011, 2011, Nantes, France. pp.409
Circumstellar disks are characteristic for star formation and vanish during the first few Myr of stellar evolution. During this time planets are believed to form in the dense midplane by growth, sedimentation and aggregation of dust. Indicators of di
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5c8f3c72799d0cefc51a0bc01e14ca2b
https://hal.archives-ouvertes.fr/hal-00702360
https://hal.archives-ouvertes.fr/hal-00702360
Publikováno v:
Astronomy & Astrophysics. 546:A7
Aims. We aim to evaluate the evolutionary stage of the circumstellar disk around DoAr 33, a T Tauri star in the Ophiuchus molecular cloud and a promising target for follow-up observations to find signs of dust evolution in protoplanetary disks.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::67ed3ee8bc5178c0488f25332ef7bd1c
https://doi.org/10.1051/0004-6361/201219336
https://doi.org/10.1051/0004-6361/201219336
Publikováno v:
Research in Astronomy & Astrophysics; Apr2013, Vol. 13 Issue 4, p420-434, 15p