Zobrazeno 1 - 10
of 1 676
pro vyhledávání: '"Fischer, W. P. P."'
Autor:
Le, N., Karska, A., Figueira, M., Sewiło, M., Mirocha, A., Fischer, Ch., Kaźmierczak-Barthel, M., Klein, R., Gawroński, M., Koprowski, M., Kowalczyk, K., Fischer, W. J., Menten, K. M., Wyrowski, F., König, C., Kristensen, L. E.
Publikováno v:
A&A 674, A64 (2023)
(abridged) Far-infrared (FIR) line emission provides key information about the gas cooling and heating due to shocks and UV radiation associated with the early stages of star formation. Gas cooling via FIR lines might, however, depend on metallicity.
Externí odkaz:
http://arxiv.org/abs/2304.08127
Autor:
Agapov, I., Benedikt, M., Blondel, A., Boscolo, M., Brunner, O., Llatas, M. Chamizo, Charles, T., Denisov, D., Fischer, W., Gianfelice-Wendt, E., Gutleber, J., Janot, P., Koratzinos, M., Losito, R., Nagaitsev, S., Oide, K., Raubenheimer, T., Rimmer, R., Seeman, J., Shatilov, D., Shiltsev, V., Sullivan, M., Wienands, U., Zimmermann, F.
The worldwide High Energy Physics community widely agrees that the next collider should be a Higgs factory. Acknowledging this priority, in 2021 CERN has launched the international Future Circular Collider (FCC) Feasibility Study (FS). The FCC Integr
Externí odkaz:
http://arxiv.org/abs/2203.08310
Autor:
Espaillat, C. C., Herczeg, G. J., Thanathibodee, T., Pittman, C., Calvet, N., Arulanantham, N., France, K., Serna, Javier, Hernandez, J., Kospal, A., Walter, F. M., Frasca, A., Fischer, W. J., Johns-Krull, C. M., Schneider, P. C., Robinson, C., Edwards, Suzan, Abraham, P., Fang, Min, Erkal, J., Manara, C. F., Alcala, J. M., Alecian, E., Alexander, R. D., Alonso-Santiago, J., Antoniucci, Simone, Ardila, David R., Banzatti, Andrea, Benisty, M., Bergin, Edwin A., Biazzo, Katia, Briceno, Cesar, Campbell-White, Justyn, Cleeves, L. Ilsedore, Coffey, Deirdre, Eisloffel, Jochen, Facchini, Stefano, Fedele, D., Fiorellino, Eleonora, Froebrich, Dirk, Gangi, Manuele, Giannini, Teresa, Grankin, K., Gunther, Hans Moritz, Guo, Zhen, Hartmann, Lee, Hillenbrand, Lynne A., Hinton, P. C., Kastner, Joel H., Koen, Chris, Mauco, K., Mendigutia, I., Nisini, B., Panwar, Neelam, Principe, D. A., Robberto, Massimo, Sicilia-Aguilar, A., Valenti, Jeff A., Wendeborn, J., Williams, Jonathan P., Xu, Ziyan, Yadav, R. K.
The Hubble UV Legacy Library of Young Stars as Essential Standards (ULLYSES) Director's Discretionary Program of low-mass pre-main-sequence stars, coupled with forthcoming data from ALMA and JWST, will provide the foundation to revolutionize our unde
Externí odkaz:
http://arxiv.org/abs/2201.06502
Autor:
Zakri, W., Megeath, S. T., Fischer, W. J., Gutermuth, Robert, Furlan, Elise, Hartmann, Lee, Karnath, Nicole, Osorio, Mayra, Safron, Emily, Stanke, Thomas, Stutz, Amelia M., Tobin, John J., Allen, Thomas S., Federman, Sam, Habel, Nolan, Manoj, P., Narang, Mayank, Pokhrel, Riwaj, Rebull, Luisa, Sheehan, Patrick D., Watson, Dan M.
At least half of a protostar's mass is accreted in the Class 0 phase, when the central protostar is deeply embedded in a dense, infalling envelope. We present the first systematic search for outbursts from Class 0 protostars in the Orion clouds. Usin
Externí odkaz:
http://arxiv.org/abs/2201.04647
Autor:
Manara, C. F., Frasca, A., Venuti, L., Siwak, M., Herczeg, G. J., Calvet, N., Hernandez, J., Tychoniec, Ł., Gangi, M., Alcalá, J. M., Boffin, H. M. J., Nisini, B., Robberto, M., Briceno, C., Campbell-White, J., Sicilia-Aguilar, A., McGinnis, P., Fedele, D., Kóspál, Á., Ábrahám, P., Alonso-Santiago, J., Antoniucci, S., Arulanantham, N., Bacciotti, F., Banzatti, A., Beccari, G., Benisty, M., Biazzo, K., Bouvier, J., Cabrit, S., Garatti, A. Caratti o, Coffey, D., Covino, E., Dougados, C., Eislöffel, J., Ercolano, B., Espaillat, C. C., Erkal, J., Facchini, S., Fang, M., Fiorellino, E., Fischer, W. J., France, K., Gameiro, J. F., Lopez, R. Garcia, Giannini, T., Ginski, C., Grankin, K., Günther, H. M., Hartmann, L., Hillenbrand, L. A., Hussain, G. A. J., James, M. M., Koutoulaki, M., Lodato, G., Maucó, K., Mendigutía, I., Mentel, R., Miotello, A., Oudmaijer, R. D., Rigliaco, E., Rosotti, G. P., Sanchis, E., Schneider, P. C., Spina, L., Stelzer, B., Testi, L., Thanathibodee, T., Vink, J. S., Walter, F. M., Williams, J. P., Zsidi, G.
Publikováno v:
A&A 650, A196 (2021)
The evolution of young stars and disks is driven by the interplay of several processes, notably accretion and ejection of material. Critical to correctly describe the conditions of planet formation, these processes are best probed spectroscopically.
Externí odkaz:
http://arxiv.org/abs/2103.12446
Autor:
Nagy, Z., Menechella, A., Megeath, S. T., Tobin, J. J., Booker, J. J., Fischer, W. J., Manoj, P., Stanke, T., Stutz, A., Wyrowski, F.
Publikováno v:
A&A 642, A137 (2020)
We aim to characterize the outflow properties of a sample of early Class 0 phase low-mass protostars in Orion first identified by the Herschel Space Observatory. We also look for signatures of infall in key molecular lines. CO $J$=3-2 and $J$=4-3 map
Externí odkaz:
http://arxiv.org/abs/2007.12103
Autor:
Lodato, G., Dipierro, G., Ragusa, E., Long, F., Herczeg, G. J., Pascucci, I., Pinilla, P., Manara, C. F., Tazzari, M., Liu, Y., Mulders, G. D., Harsono, D., Boehler, Y., Menard, F., Johnstone, D., Salyk, C., van der Plas, G., Cabrit, S., Edwards, S., Fischer, W. J., Hendler, N., Nisini, B., Rigliaco, E., Avenhaus, H., Banzatti, A., Gully-Santiago, M.
ALMA has observed a plethora of ring-like structures in planet forming discs at distances of 10-100 au from their host star. Although several mechanisms have been invoked to explain the origin of such rings, a common explanation is that they trace ne
Externí odkaz:
http://arxiv.org/abs/1903.05117
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
Rodríguez, A. K. Díaz, Osorio, M., Anglada, G., Megeath, S. T., Rodríguez, L. F., Tobin, J. J., Furlan, E., Gómez, J. F., Stutz, A. M., Fischer, W., Manoj, P., González-García, B., Stanke, T., Booker, J., Ali, B.
The nature of the far-IR source HOPS 108 has been a matter of debate in the last years. Previous radio observations detected a 3.6 cm source (VLA 12), coincident with HOPS 108, that was interpreted as a radio jet from this protostar. We present new m
Externí odkaz:
http://arxiv.org/abs/1712.00596
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.