Zobrazeno 1 - 10
of 342
pro vyhledávání: '"BLOMMAERT, J. A. D. L."'
Autor:
Fransson, C., Barlow, M. J., Kavanagh, P. J., Larsson, J., Jones, O. C., Sargent, B., Meixner, M., Bouchet, P., Temim, T., Wright, G. S., Blommaert, J. A. D. L., Habel, N., Hirschauer, A. S., Hjorth, J., Lenkić, L., Tikkanen, T., Wesson, R., Coulais, A., Fox, O. D., Gastaud, R., Glasse, A., Jaspers, J., Krause, O., Lau, R. M., Nayak, O., Rest, A., Colina, L., van Dishoeck, E. F., Gudel, M., Henning, Th., Lagage, P. -O., Őstlin, G., Ray, T. P., Vandenbussche, B.
Publikováno v:
SCIENCE 22 Feb 2024 Vol 383, Issue 6685 pp. 898-903
The nearby Supernova 1987A was accompanied by a burst of neutrino emission, which indicates that a compact object (a neutron star or black hole) was formed in the explosion. There has been no direct observation of this compact object. In this work, w
Externí odkaz:
http://arxiv.org/abs/2403.04386
Autor:
Bouchet, P., Gastaud, R., Coulais, A., Barlow, M. J., Fransson, C., Kavanagh, P. J., Larsson, J., Temim, T., Jones, O. C., Hirschauer, A. S., Tikkanen, T., Blommaert, J. A. D. L., Fox, O. D., Glasse, A., Habel, N., Hjorth, J., Jaspers, J., Krause, O., Lau, R. M., Lenkić, L., Meixner, M., Nayak, O., Rest, A., Sargent, B., Wesson, R., Wright, G. S., Colina, L., Van Dishoeck, E. F., Güdel, M., Henning, Th., Lagage, P. -O., Östlin, G., Ray, T. P., Vandenbussche, B.
There exist very few mid-infrared (IR) observations of supernovae (SNe) in general. Therefore, SN 1987A, the closest visible SN in 400 years, gives us the opportunity to explore the mid-IR properties of SNe, the dust in their ejecta and surrounding m
Externí odkaz:
http://arxiv.org/abs/2402.14014
Autor:
Jones, O. C., Kavanagh, P. J., Barlow, M. J., Temim, T., Fransson, C., Larsson, J., Blommaert, J. A. D. L., Meixner, M., Lau, R. M., Sargent, B., Bouchet, P., Hjorth, J., Wright, G. S., Coulais, A., Fox, O. D., Gastaud, R., Glasse, A., Habel, N., Hirschauer, A. S., Jaspers, J., Krause, O., Lenkić, Nayak, O., Rest, A., Tikkanen, T., Wesson, R., Colina, L., van Dishoeck, E. F., Güdel, M., Henning, Th., Lagage, P. -O., Östlin, Ray, T. P., Vandenbussche, B.
Supernova (SN) 1987A is the nearest supernova in $\sim$400 years. Using the {\em JWST} MIRI Medium Resolution Spectrograph, we spatially resolved the ejecta, equatorial ring (ER) and outer rings in the mid-infrared 12,927 days after the explosion. Th
Externí odkaz:
http://arxiv.org/abs/2307.06692
Autor:
Larsson, J., Fransson, C., Sargent, B., Jones, O. C., Barlow, M. J., Bouchet, P., Meixner, M., Blommaert, J. A. D. L., Coulais, A., Fox, O. D., Gastaud, R., Glasse, A., Habel, N., Hirschauer, A. S., Hjorth, J., Jaspers, J., Kavanagh, P. J., Krause, O., Lau, R. M., Lenkic, L., Nayak, O., Rest, A., Temim, T., Tikkanen, T., Wesson, R., Wright, G. S.
We present initial results from JWST NIRSpec integral field unit observations of the nearby Supernova (SN) 1987A. The observations provide the first spatially-resolved spectroscopy of the ejecta and equatorial ring (ER) over the 1-5 \mu m range. We c
Externí odkaz:
http://arxiv.org/abs/2302.03576
Autor:
Olofsson, H., Khouri, T., Sargent, B. A., Winnberg, A., Blommaert, J. A. D. L., Groenewegen, M. A. T., Muller, S., Kastner, J. H., Meixner, M., Otsuka, M., Patel, N., Ryde, N., Srinivasan, S.
12CO and 13CO lines, as well as a mm-wave continuum, have been observed for a sample of 22 OH/IR stars in directions within 2 degrees of the Galactic Centre. Photometry data have been gathered from the literature to construct SEDs and to determine pu
Externí odkaz:
http://arxiv.org/abs/2207.09701
The search for extrasolar planets has driven rapid advances in instrumentation, resulting in cameras such as SPHERE at the VLT, GPI at Gemini South and SCExAO at Subaru, capable of achieving very high contrast ($\sim10^{6}$) around bright stars with
Externí odkaz:
http://arxiv.org/abs/2002.04762
Autor:
Viaene, S., Baes, M., Tamm, A., Tempel, E., Bendo, G., Blommaert, J. A. D. L., Boquien, M., Boselli, A., Camps, P., Cooray, A., De Looze, I., De Vis, P., Fernandez-Ontiveros, J. A., Fritz, J., Galametz, M., Gentile, G., Madden, S., Smith, M. W. L., Spinoglio, L., Verstocken, S.
Publikováno v:
A&A 599, A64 (2017)
The radiation of stars heats dust grains in the diffuse interstellar medium and in star-forming regions in galaxies. Modelling this interaction provides information on dust in galaxies, a vital ingredient for their evolution. It is not straightforwar
Externí odkaz:
http://arxiv.org/abs/1609.08643
Autor:
Brandeker, A., Cataldi, G., Olofsson, G., Vandenbussche, B., Acke, B., Barlow, M. J., Blommaert, J. A. D. L., Cohen, M., Dent, W. R. F., Dominik, C., Di Francesco, J., Fridlund, M., Gear, W. K., Glauser, A. M., Greaves, J. S., Harvey, P. M., Heras, A. M., Hogerheijde, M. R., Holland, W. S., Huygen, R., Ivison, R. J., Leeks, S. J., Lim, T. L., Liseau, R., Matthews, B. C., Pantin, E., Pilbratt, G. L., Royer, P., Sibthorpe, B., Waelkens, C., Walker, H. J.
Publikováno v:
A&A 591, A27 (2016)
The young star beta Pictoris is well known for its dusty debris disk, produced through the grinding down by collisions of planetesimals, kilometre-sized bodies in orbit around the star. In addition to dust, small amounts of gas are also known to orbi
Externí odkaz:
http://arxiv.org/abs/1604.07418
Autor:
Lombaert, R., Decin, L., Royer, P., de Koter, A., Cox, N. L. J., González-Alfonso, E., Neufeld, D., De Ridder, J., Agúndez, M., Blommaert, J. A. D. L., Khouri, T., Groenewegen, M. A. T., Kerschbaum, F., Cernicharo, J., Vandenbussche, B., Waelkens, C.
Publikováno v:
A&A 588, A124 (2016)
Context. The recent detection of warm H$_2$O vapor emission from the outflows of carbon-rich asymptotic giant branch (AGB) stars challenges the current understanding of circumstellar chemistry. Two mechanisms have been invoked to explain warm H$_2$O
Externí odkaz:
http://arxiv.org/abs/1601.07017
Autor:
Scicluna, P., Siebenmorgen, R., Wesson, R., Blommaert, J. A. D. L, Kasper, M., Voshchinnikov, N. V., Wolf, S.
Publikováno v:
A&A 584, L10 (2015)
Massive stars live short lives, losing large amounts of mass through their stellar wind. Their mass is a key factor determining how and when they explode as supernovae, enriching the interstellar medium with heavy elements and dust. During the red su
Externí odkaz:
http://arxiv.org/abs/1511.07624