Zobrazeno 1 - 10
of 313
pro vyhledávání: '"de Winter D"'
Autor:
van der Hoeven, Jessi E. S., van der Wee, Ernest B., de Winter, D. A. Matthijs, Hermes, Michiel, Liu, Yang, Fokkema, Jantina, Bransen, Maarten, van Huis, Marijn A., Gerritsen, Hans C., de Jongh, Petra E., van Blaaderen, Alfons
Publikováno v:
Nanoscale, 2019, 11, 5304-5316
Insight in the structure of nanoparticle assemblies up to a single particle level is key to understand the collective properties of these assemblies, which critically depend on the individual particle positions and orientations. However, the characte
Externí odkaz:
http://arxiv.org/abs/1903.09989
Autor:
de Winter, D. A. Matthijs, Verhoeven, Frank M., Vermeulen, Lucie C., Duizer, Erwin, Bartels, Alvin A., de Roda Husman, Ana Maria, Schijven, Jack F.
Publikováno v:
Physics of Fluids; May2024, Vol. 36 Issue 5, p1-14, 14p
Autor:
Mora, A., Eiroa, C., Natta, A., Grady, C. A., de Winter, D., Davies, J. K., Ferlet, R., Harris, A. W., Miranda, L. F., Montesinos, B., Oudmaijer, R. D., Palacios, J., Quirrenbach, A., Rauer, H., Alberdi, A., Cameron, A., Deeg, H. J., Garzon, F., Horne, K., Merin, B., Penny, A., Schneider, J., Solano, E., Tsapras, Y., Wesselius, P. R.
Publikováno v:
Astron.Astrophys. 419 (2004) 225-240
We present high resolution (lambda / Delta_lambda = 49000) echelle spectra of the intermediate mass, pre-main sequence stars BF Ori, SV Cep, WW Wul and XY Per. The spectra cover the range 3800-5900 angstroms and monitor the stars on time scales of mo
Externí odkaz:
http://arxiv.org/abs/astro-ph/0402614
Publikováno v:
Astron.Astrophys. 416 (2004) 647-654
The southern emission-line star HD 144432 has received considerable attention due to its relative brightness (V ~ 8.17), its late spectral type (late A-type or perhaps early F) and its relative isolation from a bona-fide active star formation region.
Externí odkaz:
http://arxiv.org/abs/astro-ph/0312119
Autor:
Mora, A., Natta, A., Eiroa, C., Grady, C. A., de Winter, D., Davies, J. K., Ferlet, R., Harris, A. W., Montesinos, B., Oudmaijer, R. D., Palacios, J., Quirrenbach, A., Rauer, H., Alberdi, A., Cameron, A., Deeg, H. J., Garzon, F., Horne, K., Merin, B., Penny, A., Schneider, J., Solano, E., Tsapras, Y., Wesselius, P. R.
Publikováno v:
Astron.Astrophys. 393 (2002) 259-271
We present the results of a high spectral resolution study of the circumstellar (CS) gas around the intermediate mass, pre-main sequence star UX Ori. The results are based on a set of 10 echelle spectra, monitoring the star on time scales of months,
Externí odkaz:
http://arxiv.org/abs/astro-ph/0208322
Autor:
de Winter, D., Ancker, M. E. van den, Maira, A., Thé, P. S., Djie, H. R. E. Tjin A, Redondo, I., Eiroa, C., Molster, F. J.
We present a catalogue of previously unpublished optical and infrared photometry for a sample of 162 emission-line objects and shell stars visible from the southern hemisphere. The data were obtained between 1978 and 1997 in the Walraven (WULBV), Joh
Externí odkaz:
http://arxiv.org/abs/astro-ph/0110495
Recently, several groups of young stars in the solar neighborhood have been discovered. Given their proximity, these systems are ideally suited for detailed studies of star and planet formation. Here we report on a group of young stars associated wit
Externí odkaz:
http://arxiv.org/abs/astro-ph/0105037
Autor:
Djie, H. R. E. Tjin A, Ancker, M. E. van den, Blondel, P. F. C., Shevchenko, V. S., Ezhkova, O. V., de Winter, D., Grankin, K. N.
Publikováno v:
Mon.Not.Roy.Astron.Soc. 325 (2001) 1441
We present new high and low resolution spectroscopic and photometric data of nine members of the young association CMa R1. All the stars have circumstellar dust at some distance as could be expected from their association with reflection nebulosity.
Externí odkaz:
http://arxiv.org/abs/astro-ph/0103349
We present new optical and ultraviolet spectroscopy of the anomalous EUV emitter HD 199143 (F8V). High resolution spectra in the Halpha and Na I D wavelength regions show evidence for very rapid (a few hundred km/s) rotation of the stellar photospher
Externí odkaz:
http://arxiv.org/abs/astro-ph/0011024
The spectral and extinction properties of 14 pre-main sequence candidates in the central part of the very young open cluster NGC 6383 were investigated. None of these stars shows evidence for anomalous circumstellar extinction. However, six out of 14
Externí odkaz:
http://arxiv.org/abs/astro-ph/0006283