Zobrazeno 1 - 10
of 75
pro vyhledávání: '"Schroetter I"'
Autor:
Bouché, N. F., Wendt, M., Zabl, J., Cherrey, M., Schroetter, I., Langan, I., Muzahid, S., Schaye, J., Epinat, B., Wisotzki, L., Contini, T., Richard, J., Bacon, R., Weilbacher, P. M.
We present the design, rationale, properties and catalogs of the MusE Gas FLOw and Wind survey (MEGAFLOW), a survey of the cool gaseous halos of $z\sim1$ galaxies using low-ionization MgII absorption systems. The survey consists of 22 quasar fields s
Externí odkaz:
http://arxiv.org/abs/2411.07014
Autor:
Goicoechea, Javier R., Bourlot, J. Le, Black, J. H., Alarcón, F., Bergin, E. A., Berné, O., Bron, E., Canin, A., Chapillon, E., Chown, R., Dartois, E., Gerin, M., Habart, E., Haworth, T. J., Joblin, C., Kannavou, O., Petit, F. Le, Onaka, T., Peeters, E., Pety, J., Roueff, E., Sidhu, A., Schroetter, I., Tabone, B., Tielens, A. G. G. M., Trahin, B., Van De Putte, D., Vicente, S., Zannese, M.
Publikováno v:
A&A 689, L4 (2024)
The gas-phase abundance of carbon, x_C = C/H, and its depletion factors are essential parameters for understanding the gas and solid compositions that are ultimately incorporated into planets. The majority of protoplanetary disks are born in clusters
Externí odkaz:
http://arxiv.org/abs/2408.06279
Autor:
Elyajouri, M., Ysard, N., Abergel, A., Habart, E., Verstraete, L., Jones, A., Juvela, M., Schirmer, T., Meshaka, R., Dartois, E., Lebourlot, J., Rouille, G., Onaka, T., Peeters, E., Berne, O., Alarcon, F., Bernard-Salas, J., Buragohain, M., Cami, J., Canin, A., Chown, R., Demyk, K., Gordon, K., Kannavou, O., Kirsanova, M., Madden, S., Paladini, R., Pendleton, Y., Salama, F., Schroetter, I., Sidhu, A., Rollig, M., Trahin, B., Van De Putte, D.
Publikováno v:
A&A 685, A76 (2024)
We study the emission of dust grains within the Orion Bar - a well-known, highly far-UV (FUV)-irradiated PDR. The Orion Bar because of its edge-on geometry provides an exceptional benchmark for characterizing dust evolution and the associated driving
Externí odkaz:
http://arxiv.org/abs/2401.01221
Autor:
Epinat, B., Contini, T., Mercier, W., Ciesla, L., Lemaux, B. C., Johnson, S. D., Richard, J., Brinchmann, J., Boogaard, L. A., Carton, D., Michel-Dansac, L., Bacon, R., Krajnovic, D., Finley, H., Schroetter, I., Ventou, E., Abril-Melgarejo, V., Boselli, A., Bouché, N. F., Kollatschny, W., Kovac, K., Paalvast, M., Soucail, G., Urrutia, T., Weilbacher, P. M.
Publikováno v:
A&A, 683, A205 (2024)
We introduce the MUSE gAlaxy Groups in COSMOS (MAGIC) survey, which was built to study the impact of environment on galaxy evolution over the last 8 Gyr. It consists of 17 MUSE fields targeting 14 massive structures at intermediate redshift ($0.3
Externí odkaz:
http://arxiv.org/abs/2312.00924
Autor:
Pasquini, S., Peeters, E., Schefter, B., Khan, B., Sidhu, A., Chown, R., Cami, J., Tielens, A., Alarcon, F., Canin, A., Schroetter, I., Trahin, B., Van De Putte, D., Boersma, C., Dartois, E., Onaka, T., Candian, A., Hartigan, P., Lai, T. S. -Y., Rouille, G., Sales, D. A., Zhang, Y., Habart, E., Berne, O.
Publikováno v:
A&A 685, A77 (2024)
[Abridged] JWST observations of the Orion Bar have shown the incredible richness of PAH bands and their variation on small scales. We aim to probe the photochemical evolution of PAHs across the key zones of the photodissociation region (PDR) that is
Externí odkaz:
http://arxiv.org/abs/2311.01163
Autor:
Langan, I., Zabl, J., Bouche, N. F., Ginolfi, M., Popping, G., Schroetter, I., Wendt, M., Schaye, J., Boogaard, L., Freundlich, J., Richard, J., Matthee, J., Mercier, W., Contini, T., Guo, Y., Cherrey, M.
We study the link between gas flow events and key galaxy scaling relations: the relations between star formation rate (SFR) and stellar mass (the main sequence, MS), gas metallicity and stellar mass (the mass-metallicity relation, MZR) and gas metall
Externí odkaz:
http://arxiv.org/abs/2301.10779
Autor:
Ventou, E., Contini, T., Bouché, N., Epinat, B., Brinchmann, J., Inami, H., Richard, J., Schroetter, I., Soucail, G., Steinmetz, M., Weilbacher, P.
Publikováno v:
A&A 631, A87 (2019)
It is still a challenge to assess the merger fraction of galaxies at different cosmic epochs in order to probe the evolution of their mass assembly. Using the Illustris cosmological simulations, we investigate the relation between the separation of g
Externí odkaz:
http://arxiv.org/abs/1909.03706
Autor:
Marino, R. A., Cantalupo, S., Pezzulli, G., Lilly, S. J., Gallego, S., Mackenzie, R., Matthee, J., Brinchmann, J., Bouché, N., Feltre, A., Muzahid, S., Schroetter, I., Johnson, S. D., Nanayakkara, T.
The well-known quasar SDSS J095253.83+011421.9 (J0952+0114) at z=3.02 has one of the most peculiar spectra discovered so far, showing the presence of narrow Ly$\alpha$ and broad metal emission lines. Although recent studies have suggested that a Prox
Externí odkaz:
http://arxiv.org/abs/1906.06347
Autor:
Webb, N. A., Guérou, A., Ciambur, B., Detoeuf, A., Coriat, M., Godet, O., Barret, D., Combes, F., Contini, T., Graham, Alister W., Maccarone, T. J., Mrkalj, M., Servillat, M., Schroetter, I., Wiersema, K.
Publikováno v:
A&A 602, A103 (2017)
Aims. ESO 243-49 HLX-1, otherwise known as HLX-1, is an intermediate mass black hole (IMBH) candidate located 8" (3.7 Kpc) from the centre of the edge-on S0 galaxy ESO 243-49. How the black hole came to be associated with this galaxy, and the nature
Externí odkaz:
http://arxiv.org/abs/1704.04434
Autor:
Bouché, N., Finley, H., Schroetter, I., Murphy, M. T., Richter, P., Bacon, R., Contini, T., Richard, J., Wendt, M., Kammann, S., Epinat, B., Cantalupo, S., Straka, L. A., Schaye, J., Martin, C. L., Péroux, C., Wisotzki, L., Soto, K., Lilly, S., Carollo, C. M., Brinchmann, J., Kollatschny, W.
We use a background quasar to detect the presence of circum-galactic gas around a $z=0.91$ low-mass star forming galaxy. Data from the new Multi Unit Spectroscopic Explorer (MUSE) on the VLT show that the host galaxy has a dust-corrected star-formati
Externí odkaz:
http://arxiv.org/abs/1601.07567