Zobrazeno 1 - 10
of 30
pro vyhledávání: '"G��sten, R."'
Autor:
Pabst, C. H. M., Goicoechea, J. R., Hacar, A., Teyssier, D., Bern��, O., Wolfire, M. G., Higgins, R. D., Chambers, E. T., Kabanovic, S., G��sten, R., Stutzki, J., Kramer, C., Tielens, A. G. G. M.
The [CII] 158$��$m fine-structure line is the dominant cooling line of moderate-density photodissociation regions (PDRs) illuminated by moderately bright far-ultraviolet (FUV) radiation fields. We aim to understand the origin of [CII] emission an
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e6ba9e2e995ff9b0099c90c132d4c7db
Autor:
Pabst, C. H. M., Hacar, A., Goicoechea, J. R., Teyssier, D., Bern��, O., Wolfire, M. G., Higgins, R. D., Chambers, E. T., Kabanovic, S., G��sten, R., Stutzki, J., Kramer, C., Tielens, A. G. G. M.
The [CII] $158\,��\mathrm{m}$ fine-structure line is one of the dominant coolants of the neutral interstellar medium. It is hence one of the brightest far-infrared emission lines and can be observed not only in star-forming regions throughout the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b8963ef2a947f1651f6556c7d7773186
Autor:
Guevara, C., Stutzki, J., Ossenkopf-Okada, V., Simon, R., P��rez-Beaupuits, J. P., Beuther, H., Bihr, S., Higgins, R., Graf, U., G��sten, R.
Context. The [CII] 158 ��m far-infrared (FIR) fine-structure line is one of the most important cooling lines of the star-forming interstellar medium (ISM). High spectral resolution observations have shown complex structures in the line profiles o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b6d066543e5bbc94fb2591fec1ac7030
Autor:
G��mez-Ruiz, A. I., Gusdorf, A., Leurini, S., Menten, K. M., Takahashi, S., Wyrowski, F., G��sten, R.
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, ⟨10.1051/0004-6361/201424156⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, ⟨10.1051/0004-6361/201424156⟩
OMC-2/3 is one of the nearest embedded cluster-forming region that includes intermediate-mass protostars at early stages of evolution. A previous CO (3--2) mapping survey towards this region revealed outflow activity related to sources at different e
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::800660f7e2a949b7665a802b9f551317
http://arxiv.org/abs/1906.03522
http://arxiv.org/abs/1906.03522
Autor:
Sandell, G., Salyk, C., Ancker, M. van den, de Wit, W. -J., Chambers, E., G��sten, R., Wiesemeyer, H., Richter, H.
HH 50138 is one of the brightest B[e] stars at a distance of $\sim$ 380 pc with strong infrared excess. The star was observed in [O I] 63 $��$m and [C II] 158 $��$m with high velocity resolution with upGREAT on SOFIA. The velocity resolved [O
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::9fbe85bf11c4500e4ef61f8e9bd55444
Aims: We investigate how much of the [CII] emission in the nucleus of the nearby spiral galaxy IC 342 is contributed by PDRs and by the ionized gas. We examine the spatial variations of starburst/PDR activity and study the correlation of the [CII] li
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::61deaeaca821f3d85cb9f5822616dac2
Autor:
R��llig, M., Simon, R., G��sten, R., Stutzki, J., H��bers, H. W., Hartogh, P., Jacobs, K., Guan, X., Israel, F.
Methods: We used the dual-band receiver GREAT on board the SOFIA airborne telescope to perform observations of the [C II] 158 ��m fine-structure line at the postitions of two giant molecular clouds (GMC) in the center of IC 342 (GMCs C and E) and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::54a28e386ac77baf3438cbe2b64f3663
Microwave Kinetic Inductance Detectors (MKIDs) have great potential for large very sensitive detector arrays for use in, for example, sub-mm imaging. Being intrinsically readout in the frequency domain, they are particularly suited for frequency doma
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::894c6466d347f54783f30686b1ec8fe3
http://arxiv.org/abs/0903.2431
http://arxiv.org/abs/0903.2431
Myrmica specioides Bondroit, 1918 Myrmica specioides Bondroit, 1918 Tetramorium silvestrianum Emery, 1924: syn. nov. Myrmica rugulosoides var. striata Finzi, 1926 (synonymy: Collingwood 1979) Myrmica scabrinodis var. ahngeri Karavaiev, 1926 (synonymy
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c35c5f239c03a8e28eb260f2f35d7e06
Tetramorium forte France, Dept. Vaucluse, 7 km n Avignon; Spain, Prov. Cuenca, 2 km e Villalba de la Sierra; Spain, Prov. Jaen, Puerto de los Jardines; Spain, Prov. Granada, Sierra Nevada (2200m); Spain, Prov. Badajoz, Embalse de Orellana; Portugal,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5ba9dbf80e8f473f296451dd7359b5c2