Zobrazeno 1 - 10
of 1 087
pro vyhledávání: '"Lisenfeld, U."'
Autor:
Pérez, I., Verley, S., Sánchez-Menguiano, L., Ruiz-Lara, T., García-Benito, R., Puertas, S. Duarte, Jiménez, A., Domínguez-Gómez, J., Espada, D., Peletier, R. F., Román, J., Rodríguez, M. I., Alarcón, P. Sánchez, Argudo-Fernández, M., Torres-Ríos, G., Bidaran, B., Alcázar-Laynez, M., van de Weygaert, R., Sánchez, S. F., Lisenfeld, U., Zurita, A., Florido, E., van der Hulst, J. M., Blázquez-Calero, G., Villalba-González, P., del Moral-Castro, I., Lugo-Aranda, A., Walo-Martín, D., Conrado, A., Delgado, R. González, Falcón-Barroso, J., Ferré-Mateu, A., Hernández-Sánchez, M., Awad, P., Kreckel, K., Courtois, H., Espada-Miura, R., Relaño, M., Galbany, L., Sánchez-Blázquez, P., Pérez-Montero, E., Sánchez-Portal, M., Bongiovanni, A., Planelles, S., Quilis, V., Aubert, M., Guinet, D., Pomaréde, D., Weijmans, A. M., Raj, M. A., Aragón-Calvo, M. A., Azzaro, M., Bergond, G., Blazek, M., Cikota, S., Fernández-Martín, A., Gardini, A., Guijarro, A., Hermelo, I., Martín, P., Linares, J. I. Vico
We have learnt in the last decades that the majority of galaxies belong to high density regions interconnected in a sponge-like fashion. This large-scale structure is characterised by clusters, filaments, walls, where most galaxies concentrate, but a
Externí odkaz:
http://arxiv.org/abs/2405.04217
Autor:
Domínguez-Gómez, J., Pérez, I., Ruiz-Lara, T., Peletier, R. F., Sánchez-Blázquez, P., Lisenfeld, U., Falcón-Barroso, J., Alcázar-Laynez, M., Argudo-Fernández, M., Blázquez-Calero, G., Courtois, H., Puertas, S. Duarte, Espada, D., Florido, E., García-Benito, R., Jiménez, A., Kreckel, K., Relaño, M., Sánchez-Menguiano, L., van der Hulst, T., van de Weygaert, R., Verley, S., Zurita, A.
Galaxies in the Universe are distributed in a web-like structure characterised by different large-scale environments: dense clusters, elongated filaments, sheetlike walls, and under-dense regions, called voids. The low density in voids is expected to
Externí odkaz:
http://arxiv.org/abs/2306.16818
Autor:
Cheng, Cheng, Xu, Cong Kevin, Appleton, P. N., Duc, P. -A., Tang, N. -Y., Dai, Y. S., Huang, J. -S., Lisenfeld, U., Renaud, F., He, Chuan, Feng, Hai-Cheng
We carried out deep mapping observations of the atomic hydrogen (HI) 21 cm line emission in a field centered on the famous galaxy group Stephan's Quintet (SQ), using the Five-hundred-meter Aperture Spherical Telescope (FAST) equipped with the 19-Beam
Externí odkaz:
http://arxiv.org/abs/2306.11231
Autor:
Grajales-Medina, D., Argudo-Fernández, M., Vásquez-Bustos, P., Verley, S., Boquien, M., Salim, S., Puertas, S. Duarte, Lisenfeld, U., Espada, D., Salas-Olave, H.
Publikováno v:
A&A 669, A23 (2023)
The merging system SIT 45 (UGC 12589) is an unusual isolated galaxy triplet, consisting of three merging late-type galaxies, out of 315 systems in the SIT (SDSS-based catalogue of Isolated Triplets). The main aims of this work are to study its dynami
Externí odkaz:
http://arxiv.org/abs/2209.12850
Autor:
Xu, C. K., Cheng, C., Appleton, P. N., Duc, P. -A., Gao, Y., Tang, N. -Y., Yun, M., Dai, Y. S., Huang, J. -S., Lisenfeld, U., Renaud, F.
Stephan's Quintet (SQ, distance=85$\pm$6 Mpc) is unique among compact groups of galaxies. Observations have previously shown that interactions between multiple members, including a high-speed intruder galaxy currently colliding into the intragroup me
Externí odkaz:
http://arxiv.org/abs/2208.04870
Autor:
Relano, M., De Looze, I., Saintonge, A., Hou, K. -C., Romano, L., Nagamine, K., Hirashita, H., Aoyama, S., Lamperti, I., Lisenfeld, U., Smith, M., Chastenet, J., Xiao, T., Gao, Y., Sargent, M., van der Giessen, S. A.
The evolution of the dust grain size distribution has been studied in recent years with great detail in cosmological hydrodynamical simulations taking into account all the channels under which dust evolves in the interstellar medium. We present a sys
Externí odkaz:
http://arxiv.org/abs/2207.13196
Autor:
Appleton, P. N., Emonts, B., Lisenfeld, U., Falgarone, E., Guillard, P., Boulanger, F., Braine, J., Ogle, P., Struck, C., Vollmer, B., Yeager, T.
We present ALMA observations at a spatial resolution of 0.2 arcsec (60 pc) of CO emission from the Taffy galaxies (UGC 12914/5). The observations are compared with narrow-band Pa$\alpha$, mid-IR, radio continuum and X-ray imaging, plus optical spectr
Externí odkaz:
http://arxiv.org/abs/2203.17142
Autor:
Domínguez-Gómez, J., Lisenfeld, U., Pérez, I., López-Sánchez, Á. R., Puertas, S. Duarte, Falcón-Barroso, J., Kreckel, K., Peletier, R. F., Ruiz-Lara, T., van de Weygaert, R., van der Hulst, J. M., Verley, S.
Publikováno v:
A&A 658, A124 (2022)
We present the first molecular gas mass survey of void galaxies. We compare these new data together with data for the atomic gas mass and star formation rate ($\rm SFR$) from the literature to those of galaxies in filaments and walls in order to bett
Externí odkaz:
http://arxiv.org/abs/2111.06844
Autor:
Querejeta, M., Lelli, F., Schinnerer, E., Colombo, D., Lisenfeld, U., Mundell, C. G., Bigiel, F., García-Burillo, S., Herrera, C. N., Hughes, A., Kruijssen, J. M. D., Meidt, S. E., Moore, T. J. T., Pety, J., Rigby, A. J.
Publikováno v:
A&A 645, A97 (2021)
Tidal dwarf galaxies (TDGs) are gravitationally bound condensations of gas and stars formed during galaxy interactions. Here we present multi-configuration ALMA observations of J1023+1952, a TDG in the interacting system Arp 94, where we resolve CO(2
Externí odkaz:
http://arxiv.org/abs/2011.01287
Publikováno v:
A&A 636, A18 (2020)
Dust is formed out of stellar material and is constantly affected by different mechanisms occurring in the ISM. Dust grains behave differently under these mechanisms depending on their sizes, and therefore the dust grain size distribution also evolve
Externí odkaz:
http://arxiv.org/abs/2002.01945