Zobrazeno 1 - 10
of 501
pro vyhledávání: '"Bruderer S"'
Publikováno v:
Drug Design, Development and Therapy, Vol 2015, Iss default, Pp 175-185 (2014)
Matthias Hoch,1 Borje Darpo,2,3 Tatiana Remenova,4 Randall Stoltz,5 Meijian Zhou,2 Priska Kaufmann,1 Shirin Bruderer,1 Jasper Dingemanse1 1Department of Clinical Pharmacology, Actelion Pharmaceuticals Ltd, Allschwil, Switzerland; 2iCardiac Technologi
Externí odkaz:
https://doaj.org/article/aed810519b1848f6b0a2585bd85ec052
Autor:
Pirovano, L. M., Fedele, D., van Dishoeck, E. F., Hogerheijde, M. R., Lodato, G., Bruderer, S.
[Abridged] Far-infrared observations with Herschel revealed a surprisingly low abundance of cold-water reservoirs in protoplanetary discs. On the other hand, a handful of discs show emission of hot water transitions excited at temperatures above a fe
Externí odkaz:
http://arxiv.org/abs/2207.10744
Autor:
Leemker, M., Booth, A. S., van Dishoeck, E. F., Pérez-Sánchez, A. F., Szulágyi, J., Bosman, A. D., Bruderer, S., Facchini, S., Hogerheijde, M. R., Paneque-Carreño, T., Sturm, J. A.
Publikováno v:
A&A 663, A23 (2022)
[Abridged] Most disks observed at high angular resolution show substructures. Knowledge about the gas surface density and temperature is essential to understand these. The aim of this work is to constrain the gas temperature and surface density in tw
Externí odkaz:
http://arxiv.org/abs/2204.03666
Autor:
Trapman, L., Ansdell, M., Hogerheijde, M. R., Facchini, S., Manara, C. F., Miotello, A., Williams, J. P., Bruderer, S.
Publikováno v:
A&A 638, A38 (2020)
Recent ALMA surveys of protoplanetary disks have shown that for most disks the extent of the gas emission is greater than the extent of the thermal emission of the millimeter-sized dust. Both line optical depth and the combined effect of radially dep
Externí odkaz:
http://arxiv.org/abs/2004.07257
Autor:
Kama, M., Trapman, L., Fedele, D., Bruderer, S., Hogerheijde, M. R., Miotello, A., van Dishoeck, E. F., Clarke, C., Bergin, E. A.
Publikováno v:
A&A 634, A88 (2020)
Hydrogen deuteride (HD) rotational line emission can provide reliable protoplanetary disk gas mass measurements, but it is difficult to observe and detections have been limited to three T-Tauri disks. No new data have been available since the \emph{H
Externí odkaz:
http://arxiv.org/abs/1912.11883
The extent of the gas in protoplanetary disks is observed to be universally larger than the extent of the dust. This is often attributed to radial drift and grain growth of the mm grains, but line optical depth produces a similar observational signat
Externí odkaz:
http://arxiv.org/abs/1903.06190
Autor:
Schmid, N., Bruderer, S., Paruzzo, F., Fischetti, G., Toscano, G., Graf, D., Fey, M., Henrici, A., Ziebart, V., Heitmann, B., Grabner, H., Wegner, J.D., Sigel, R.K.O., Wilhelm, D.
Publikováno v:
In Journal of Magnetic Resonance February 2023 347
Autor:
González-Alfonso, E., Fischer, J., Bruderer, S., Ashby, M. L. N., Smith, H. A., Veilleux, S., Müller, H. S. P., Stewart, K. P., Sturm, E.
The oxygen-bearing molecular ions OH+, H2O+, and H3O+ are key species that probe the ionization rate of (partially) molecular gas that is ionized by X-rays and cosmic rays permeating the interstellar medium. We report Herschel far-infrared and submil
Externí odkaz:
http://arxiv.org/abs/1803.04690
Autor:
Carney, M. T., Fedele, D., Hogerheijde, M. R., Favre, C., Walsh, C., Bruderer, S., Miotello, A., Murillo, N. M., Klaassen, P. D., Henning, Th., van Dishoeck, E. F.
Publikováno v:
A&A 614, A106 (2018)
This work aims to understand which midplane conditions are probed by the DCO$^+$ emission in the disk around the Herbig Ae star HD 169142. We explore the sensitivity of the DCO$^+$ formation pathways to the gas temperature and the CO abundance. The D
Externí odkaz:
http://arxiv.org/abs/1802.09280
Protoplanetary discs around brown dwarfs and very low mass stars offer some of the best prospects for forming Earth-sized planets in their habitable zones. To this end, we study the nature of the disc around the very low mass star V410 X-ray 1, whose
Externí odkaz:
http://arxiv.org/abs/1802.07120