Zobrazeno 1 - 10
of 715
pro vyhledávání: '"Pawellek A"'
Autor:
Arabhavi, A. M., Kamp, I., Henning, Th., van Dishoeck, E. F., Christiaens, V., Gasman, D., Perrin, A., Güdel, M., Tabone, B., Kanwar, J., Waters, L. B. F. M., Pascucci, I., Samland, M., Perotti, G., Bettoni, G., Grant, S. L., Lagage, P. O., Ray, T. P., Vandenbussche, B., Absil, O., Argyriou, I., Barrado, D., Boccaletti, A., Bouwman, J., Garatti, A. Caratti o, Glauser, A. M., Lahuis, F., Mueller, M., Olofsson, G., Pantin, E., Scheithauer, S., Morales-Calderón, M., Franceschi, R., Jang, H., Pawellek, N., Rodgers-Lee, D., Schreiber, J., Schwarz, K., Temmink, M., Vlasblom, M., Wright, G., Colina, L., Östlin, G.
Publikováno v:
Science, Vol 384, Issue 6700, 2024, pp. 1086-1090
Very low-mass stars (those <0.3 solar masses) host orbiting terrestrial planets more frequently than other types of stars, but the compositions of those planets are largely unknown. We use mid-infrared spectroscopy with the James Webb Space Telescope
Externí odkaz:
http://arxiv.org/abs/2406.14293
Autor:
Besginow, Andreas, Hüwel, Jan David, Pawellek, Thomas, Beecks, Christian, Lange-Hegermann, Markus
Model selection aims to find the best model in terms of accuracy, interpretability or simplicity, preferably all at once. In this work, we focus on evaluating model performance of Gaussian process models, i.e. finding a metric that provides the best
Externí odkaz:
http://arxiv.org/abs/2403.09215
Autor:
Henning, Thomas, Kamp, Inga, Samland, Matthias, Arabhavi, Aditya M., Kanwar, Jayatee, van Dishoeck, Ewine F., Guedel, Manuel, Lagage, Pierre-Olivier, Waelkens, Christoffel, Abergel, Alain, Absil, Olivier, Barrado, David, Boccaletti, Anthony, Bouwman, Jeroen, Garatti, Alessio Caratti o, Geers, Vincent, Glauser, Adrian M., Lahuis, Fred, Nehme, Cyrine, Olofsson, Goeran, Pantin, Eric, Ray, Tom P., Vandenbussche, Bart, Waters, L. B. F. M., Wright, Gillian, Christiaens, Valentin, Franceschi, Riccardo, Gasman, Danny, Guadarrama, Rodrigo, Jang, Hyerin, Morales-Calderon, Maria, Pawellek, Nicole, Perotti, Giulia, Rodgers-Lee, Donna, Schreiber, Juergen, Schwarz, Kamber, Tabone, Benoit, Temmink, Milou, Vlasblom, Marissa, Colina, Luis, Greve, Thomas R., Oestlin, Goeran
The study of protoplanetary disks has become increasingly important with the Kepler satellite finding that exoplanets are ubiquitous around stars in our galaxy and the discovery of enormous diversity in planetary system architectures and planet prope
Externí odkaz:
http://arxiv.org/abs/2403.09210
Autor:
Ginski, C., Garufi, A., Benisty, M., Tazaki, R., Dominik, C., Ribas, A., Engler, N., Birnstiel, T., Chauvin, G., Columba, G., Facchini, S., Goncharov, A., Hagelberg, J., Henning, T., Hogerheijde, M., van Holstein, R. G., Huang, J., Muto, T., Pinilla, P., Kanagawa, K., Kim, S., Kurtovic, N., Langlois, M., Manara, C., Milli, J., Momose, M., Orihara, R., Pawellek, N., Pinte, C., Rab, C., Schmidt, T. O. B., Snik, F., Wahhaj, Z., Williams, J., Zurlo, A.
We used VLT/SPHERE to observe 20 systems in the Cha I cloud in polarized scattered light in the near-infrared. We combined the scattered light observations with existing literature data on stellar properties and with archival ALMA continuum data to s
Externí odkaz:
http://arxiv.org/abs/2403.02149
Autor:
Moór, A., Ábrahám, P., Su, K. Y. L., Henning, T., Marino, S., Chen, L., Kóspál, Á., Pawellek, N., Varga, J., Vida, K.
Publikováno v:
Monthly Notices of the Royal Astronomical Society, Volume 528, Issue 3, March 2024, pp.4528-4546
Extreme debris discs (EDDs) are bright and warm circumstellar dusty structures around main sequence stars. They may represent the outcome of giant collisions occuring in the terrestrial region between large planetesimals or planetary bodies, and thus
Externí odkaz:
http://arxiv.org/abs/2402.15438
Autor:
Pawellek, Nicole, Moór, Attila, Kirchschlager, Florian, Milli, Julien, Kóspál, Agnes, Abrahám, Péter, Marino, Sebastian, Wyatt, Mark, Rebollido, Isabel, Hughes, A. Meredith, Cantalloube, Faustine, Henning, Thomas
We show the first SPHERE/IRDIS and IFS data of the CO-rich debris disc around HD 131488. We use N-body simulations to model both the scattered light images and the SED of the disc in a self-consistent way. We apply the Henyey-Greenstein approximation
Externí odkaz:
http://arxiv.org/abs/2311.03272
Autor:
Maja Pawellek, Angela Köninger, Michael Melter, Michael Kabesch, Christian Apfelbacher, Susanne Brandstetter, KUNO-Kids study group
Publikováno v:
BMC Public Health, Vol 24, Iss 1, Pp 1-13 (2024)
Abstract Background Parents can engage in several behaviours with regard to early childhood allergy prevention (ECAP). These can be related to diet of mother/child and the modification of the home environment; not all of them are justified by current
Externí odkaz:
https://doaj.org/article/d1a203c8614544aa84e93cba432bbf91
Autor:
Kamp, Inga, Henning, Thomas, Arabhavi, Aditya M., Bettoni, Giulio, Christiaens, Valentin, Gasman, Danny, Grant, Sierra L., Morales-Calderón, Maria, Tabone, Benoît, Abergel, Alain, Absil, Olivier, Argyriou, Ioannis, Barrado, David, Boccaletti, Anthony, Bouwman, Jeroen, Garatti, Alessio Caratti o, van Dishoeck, Ewine F., Geers, Vincent, Glauser, Adrian M., Güdel, Manuel, Guadarrama, Rodrigo, Jang, Hyerin, Kanwar, Jayatee, Lagage, Pierre-Olivier, Lahuis, Fred, Mueller, Michael, Nehmé, Cyrine, Olofsson, Göran, Pantin, Eric, Pawellek, Nicole, Perotti, Giulia, Ray, Tom P., Rodgers-Lee, Donna, Samland, Matthias, Scheithauer, Silvia, Schreiber, Jürgen, Schwarz, Kamber, Temmink, Milou, Vandenbussche, Bart, Vlasblom, Marissa, Waelkens, Christoffel, Waters, L. B. F. M., Wright, Gillian
The understanding of planet formation has changed recently, embracing the new idea of pebble accretion. This means that the influx of pebbles from the outer regions of planet-forming disks to their inner zones could determine the composition of plane
Externí odkaz:
http://arxiv.org/abs/2307.16729
Autor:
Perotti, G., Christiaens, V., Henning, Th., Tabone, B., Waters, L. B. F. M., Kamp, I., Olofsson, G., Grant, S. L., Gasman, D., Bouwman, J., Samland, M., Franceschi, R., van Dishoeck, E. F., Schwarz, K., Güdel, M., Lagage, P. -O., Ray, T. P., Vandenbussche, B., Abergel, A., Absil, O., Arabhavi, A. M., Argyriou, I., Barrado, D., Boccaletti, A., Garatti, A. Caratti o, Geers, V., Glauser, A. M., Justannont, K., Lahuis, F., Mueller, M., Nehmé, C., Pantin, E., Scheithauer, S., Waelkens, C., Guadarrama, R., Jang, H., Kanwar, J., Morales-Calderón, M., Pawellek, N., Rodgers-Lee, D., Schreiber, J., Colina, L., Greve, T. R., Östlin, G., Wright, G.
Terrestrial and sub-Neptune planets are expected to form in the inner ($<10~$AU) regions of protoplanetary disks. Water plays a key role in their formation, although it is yet unclear whether water molecules are formed in-situ or transported from the
Externí odkaz:
http://arxiv.org/abs/2307.12040
Autor:
Gasman, Danny, van Dishoeck, Ewine F., Grant, Sierra L., Temmink, Milou, Tabone, Benoît, Henning, Thomas, Kamp, Inga, Güdel, Manuel, Lagage, Pierre-Olivier, Perotti, Giulia, Christiaens, Valentin, Samland, Matthias, Arabhavi, Aditya M., Argyriou, Ioannis, Abergel, Alain, Absil, Olivier, Barrado, David, Boccaletti, Anthony, Bouwman, Jeroen, Garatti, Alessio Caratti o, Geers, Vincent, Glauser, Adrian M., Guadarrama, Rodrigo, Jang, Hyerin, Kanwar, Jayatee, Lahuis, Fred, Morales-Calderón, Maria, Mueller, Michael, Nehmé, Cyrine, Olofsson, Göran, Pantin, Eric, Pawellek, Nicole, Ray, Tom P., Rodgers-Lee, Donna, Scheithauer, Silvia, Schreiber, Jürgen, Schwarz, Kamber, Vandenbussche, Bart, Vlasblom, Marissa, Waters, L. B. F. M., Wright, Gillian, Colina, Luis, Greve, Thomas R., Östlin, Göran
MIRI/MRS on board the JWST allows us to probe the inner regions of protoplanetary disks. Here we examine the disk around the classical T Tauri star Sz 98, which has an unusually large dust disk in the millimetre with a compact core. We focus on the H
Externí odkaz:
http://arxiv.org/abs/2307.09301