Zobrazeno 1 - 10
of 858
pro vyhledávání: '"Buchbender A"'
Autor:
Keilmann, Eduard, Kabanovic, Slawa, Schneider, Nicola, Ossenkopf-Okada, Volker, Stutzki, Jürgen, Kobayashi, Masato I. N., Simon, Robert, Buchbender, Christof, Riechers, Dominik, Bigiel, Frank, Tabatabaei, Fatemeh
Understanding mass, size, and surface mass density of giant molecular clouds (GMCs) in galaxies is key to insights into star formation processes. We analyze these in M33 using Herschel dust and archival IRAM 30m telescope data, compared to Milky Way
Externí odkaz:
http://arxiv.org/abs/2411.10806
Autor:
Okada, Yoko, Kabanovic, Slawa, Güsten, Rolf, Ossenkopf-Okada, Volker, Schneider, Nicola, Simon, Robert, Buchbender, Christof, Higgins, Ronan, Yanitski, Craig, Röllig, Markus, Stutzki, Jürgen, Ishihara, Daisuke, Tanaka, Kunihiko, Chambers, Edward, Honingh, Netty, Justen, Matthias, Riquelme, Denise
We investigate the dynamical and physical structures of bright-rimmed clouds (BRCs) in a nearby HII region. We focused on carbon- and oxygen-bearing species that trace photon-dominated regions (PDRs) and warm molecular cloud surfaces in order to unde
Externí odkaz:
http://arxiv.org/abs/2408.12432
Autor:
Keilmann, Eduard, Buchbender, Christof, Ossenkopf-Okada, Volker, Schneider, Nicola, Kabanovic, Slawa, Stutzki, Jürgen, Simon, Robert, Riechers, Dominik, Tabatabaei, Fateneh, Bigiel, Frank
This study is aimed to contribute to a more comprehensive understanding of the molecular hydrogen distribution in the galaxy M33 by introducing novel methods for generating high angular resolution (18.2$''$, equivalent to 75 pc) column density maps o
Externí odkaz:
http://arxiv.org/abs/2406.03601
Autor:
Bonne, L., Kabanovic, S., Schneider, N., Zavagno, A., Keilmann, E., Simon, R., Buchbender, C., Guesten, R., Jacob, A. M., Jacobs, K., Kavak, U., Polles, F. L., Tiwari, M., Wyrowski, F., Tielens, A. G. G. M
Publikováno v:
A&A 679, L5 (2023)
It has long been discussed whether stellar feedback in the form of winds and/or radiation can shred the nascent molecular cloud, thereby controlling the star formation rate. However, directly probing and quantifying the impact of stellar feedback on
Externí odkaz:
http://arxiv.org/abs/2310.01657
Autor:
Daniel Einsiedel, Stephanie Knapp Giacaman, Anna Seidel, Lara Berger, Mayte Buchbender, Manfred Wichmann, Ragai Edward Matta
Publikováno v:
BMC Medical Education, Vol 24, Iss 1, Pp 1-12 (2024)
Abstract Background This in vitro study investigated whether full-guided (FG) or half-guided (HG) implant placement is more suitable for beginners and to what extent the use of the coDiagnostiX (CDX) (10.5, Straumann Group, Basel, Switzerland) implan
Externí odkaz:
https://doaj.org/article/0aa887002e044206afd24faf40371002
Autor:
Schneider, Nicola, Bonne, Lars, Bontemps, Sylvain, Kabanovic, Slawa, Simon, Robert, Ossenkopf-Okada, Volker, Buchbender, Christof, Stutzki, Juergen, Mertens, Marc, Ricken, Oliver, Csengeri, Timea, Tielens, Alexander G. G. M.
Molecular hydrogen clouds are a key component of the interstellar medium because they are the birthplaces for stars. They are embedded in atomic gas that pervades the interstellar space. However, the details of how molecular clouds assemble from and
Externí odkaz:
http://arxiv.org/abs/2302.09266
Autor:
Tiwari, M., Wolfire, M., Pound, M. W., Tarantino, E., Karim, R., Bonne, L., Buchbender, C., Güsten, R., Guevara, C., Kabanovic, S., Kavak, Ü., Mertens, M., Schneider, N., Simon, R., Stutzki, J., Tielens, A. G. G. M.
We quantified the effects of stellar feedback in RCW 49 by determining the physical conditions in different regions using the [CII] 158 $\mu$m and [OI] 63 $\mu$m observations from SOFIA, the $^{12}$CO (3-2) observations from APEX and the H$_2$ line o
Externí odkaz:
http://arxiv.org/abs/2208.08174
Autor:
Bonne, L., Schneider, N., García, P., Bij, A., Broos, P., Fissel, L., Guesten, R., Jackson, J., Simon, R., Townsley, L., Zavagno, A., Aladro, R., Buchbender, C., Guevara, C., Higgins, R., Jacob, A. M., Kabanovic, S., Karim, R., Soam, A., Stutzki, J., Tiwari, M., Wyrowski, F., Tielens, A. G. G. M.
We present [CII] 158 $\mu$m and [OI] 63 $\mu$m observations of the bipolar HII region RCW 36 in the Vela C molecular cloud, obtained within the SOFIA legacy project FEEDBACK, which is complemented with APEX $^{12/13}$CO(3-2) and Chandra X-ray (0.5-7
Externí odkaz:
http://arxiv.org/abs/2207.06479
Autor:
Beuther, H., Schneider, N., Simon, R., Suri, S., Ossenkopf-Okada, V., Kabanovic, S., Roellig, M., Guevara, C., Tielens, A. G. G. M., Sandell, G., Buchbender, C., Ricken, O., Guesten, R.
Publikováno v:
A&A 659, A77 (2022)
Context: How do expanding HII regions interact with their environmental cloud? This is one of the central questions driving the SOFIA legacy program FEEDBACK. Here, we present a case study toward the prototypical H{\sc ii} region NGC7538. Methods: Wi
Externí odkaz:
http://arxiv.org/abs/2201.05532
Autor:
Kabanovic, S., Schneider, N., Ossenkopf-Okada, V., Falasca, F., Güsten, R., Stutzki, J., Simon, R., Buchbender, C., Anderson, L., Bonne, L., Guevara, C., Higgins, R., Koribalski, B., Luisi, M., Mertens, M., Okada, Y., Röllig, M., Seifried, D., Tiwari, M., Wyrowski, F., Zavagno, A., Tielens, A. G. G. M.
Publikováno v:
A&A 659, A36 (2022)
Revealing the 3D dynamics of HII regions and their associated molecular clouds is important for understanding the longstanding problem as to how stellar feedback affects the density structure and kinematics of the interstellar medium. We employed obs
Externí odkaz:
http://arxiv.org/abs/2112.11336