Zobrazeno 1 - 10
of 17
pro vyhledávání: '"Schreyer, Katharina"'
Autor:
Dutrey, Anne, Wakelam, Valentine, Boehler, Yann, Guilloteau, Stéphane, Hersant, Franck, Semenov, Dmitry, Chapillon, Edwige, Henning, Thomas, Piétu, Vincent, Launhardt, Ralf, Gueth, Frederic, Schreyer, Katharina
We study the content in S-bearing molecules of protoplanetary disks around low-mass stars. We used the new IRAM 30-m receiver EMIR to perform simultaneous observations of the $1_{10}-1_{01}$ line of H$_2$S at 168.8 GHz and $2_{23}-1_{12}$ line of SO
Externí odkaz:
http://arxiv.org/abs/1109.5870
Autor:
Forbrich, Jan, Stanke, Thomas, Klein, Randolf, Henning, Thomas, Menten, Karl M., Schreyer, Katharina, Posselt, Bettina
(abridged) We study a previously discovered protostellar source that is deeply embedded and drives an energetic molecular outflow. The source, UYSO1, is located close to IRAS 07029-1215 at a distance of ~1 kpc. The multi-wavelength observations resul
Externí odkaz:
http://arxiv.org/abs/0809.5048
Autor:
Schreyer, Katharina, Guilloteau, Stéphane, Semenov, Dmitry, Bacmann, Aurore, Chapillon, Edwige, Dutrey, Anne, Gueth, Frederic, Henning, Thomas, Hersant, Frank, Launhardt, Ralf, Pety, Jerome, Pietu, Vincent
We study the molecular content and chemistry of a circumstellar disk surrounding the Herbig Ae star AB Aur at (sub-)millimeter wavelengths. Our aim is to reconstruct the chemical history and composition of the AB Aur disk and to compare it with disks
Externí odkaz:
http://arxiv.org/abs/0809.3473
Autor:
Scholz, Alexander, Jayawardhana, Ray, Wood, Kenneth, Lafreniere, David, Schreyer, Katharina, Doyon, Rene
IRAS04325+2402C is a low luminosity object located near a protostar in Taurus. We present new spatially-resolved mm observations, near-infrared spectroscopy, and Spitzer photometry that improve the constraints on the nature of this source. The object
Externí odkaz:
http://arxiv.org/abs/0806.2318
Autor:
Dutrey, Anne, Henning, Thomas, Guilloteau, Stephane, Semenov, Dmitry, Pietu, Vincent, Schreyer, Katharina, Bacmann, Aurore, Launhardt, Ralf, Pety, Jerome, Gueth, Frederic
Aims: To constrain the ionization fraction in protoplanetary disks, we present new high-sensitivity interferometric observations of N$_2$H$^+$ in three disks surrounding DM Tau, LkCa 15, and MWC 480. Methods: We used the IRAM PdBI array to observe th
Externí odkaz:
http://arxiv.org/abs/astro-ph/0612534
We present submillimeter (CSO 350um) and millimeter (SEST 1.2 mm, OVRO 3 mm) photometry for 125 solar-type stars from the FEPS Spitzer Legacy program that have masses between ~0.5 and 2.0 Msun and ages from 3 Myr to 3 Gyr. Continuum emission was dete
Externí odkaz:
http://arxiv.org/abs/astro-ph/0411020
Publikováno v:
Astrophys.J. 602 (2004) 843-849
In the course of a comprehensive mm/submm survey of massive star-forming regions, the vicinities of a sample of 47 luminous IRAS sources were closely investigated with SCUBA and IRAM bolometers in order to search for massive protostellar candidates.
Externí odkaz:
http://arxiv.org/abs/astro-ph/0311210
Publikováno v:
Astrophys.J. 599 (2003) 335-341
We present a high-resolution study of NGC 2264 IRS1 in CS(2-1) and in the 3-mm continuum using the IRAM Plateau de Bure Interferometer. We complement these radio data with images taken at 2.2, 4.6, and 11.9 micron. The combined information allow a ne
Externí odkaz:
http://arxiv.org/abs/astro-ph/0311156
Autor:
Chapillon, E., Dutrey, Anne, Henning, Thomas, Guilloteau, S., Wakelam, Valentine, Hersant, F., Gueth, Frédéric, Piétu, Vincent, Ohashi, Nagayoshi, Boehler, Y., Launhardt, Ralf, Semenov, Dimitry, Schreyer, Katharina, Guélin, Michel, Parise, Bérengère
Publikováno v:
Protostars and Planets VI, Heidelberg, July 15-20, 2013. Poster #2S023
Protostars and Planets VI, Heidelberg, July 15-20, 2013. Poster #2S023, 2013, Heidelberg, Germany
Protostars and Planets VI, Heidelberg, July 15-20, 2013. Poster #2S023, 2013, Heidelberg, Germany
We summarize in this poster a long-term study of the chemistry as a powerful tool to constrain the protoplanetary disk physics. Most of the above results were obtained in the frame of the CID (Chemistry In Disks) consortium.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::843f28cea19bfee6e4a1968c131404b2
https://hal.archives-ouvertes.fr/hal-00880565
https://hal.archives-ouvertes.fr/hal-00880565
Autor:
DUTREY, Anne, GUILLOTEAU, S., PIÉTU, V., CHAPILLON, E., GUETH, F., HENNING, T., LAUNHARDT, R., SCHREYER, Katharina, SEMENOV, D.
Publikováno v:
Bulletin of the American Astronomical Society-2008DPS....40.1107D
2008, France. pp.402
2008, France. pp.402
International audience; Recent modeling based on unresolved infrared observations of the spectral energy distribution (SED) of GM Aurigae suggests that the inner disk of this single TTauri star is truncated at an inner radius of 25 AU. Using the IRAM
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::d99b8524cd59578634dba996a1137182
https://hal.archives-ouvertes.fr/hal-00401941
https://hal.archives-ouvertes.fr/hal-00401941