Zobrazeno 1 - 10
of 19
pro vyhledávání: '"Lisenfeld, U."'
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:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6df8d7dc039e468bfad259aa727697a0
http://arxiv.org/abs/2203.17142
http://arxiv.org/abs/2203.17142
Autor:
Appleton, P. N., Guillard, P., Togi, A., Alatalo, K., Boulanger, F., Cluver, M., Pineau des Forêts, G., Lisenfeld, U., Ogle, P., Xu, C. K.
We map for the first time the two-dimensional H_2 excitation of warm intergalactic gas in Stephan's Quintet on group-wide (50 × 35 kpc^2) scales to quantify the temperature, mass, and warm H_2 mass fraction as a function of position using Spitzer. M
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od________38::d056d64532e909a3e7e0413d25bdc0d4
https://resolver.caltech.edu/CaltechAUTHORS:20170210-135050275
https://resolver.caltech.edu/CaltechAUTHORS:20170210-135050275
Autor:
Lisenfeld, U., Pérez-Torres, Miguel A., Alberdi, Antxón, Colina, Luis, García-Burillo, S., Alonso-Herrero, A.
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
The tightness and universality of the far-infrared (FIR) to radio continuum (RC) correlation is still not completely understood. This correlation is followed by all star-forming galaxies not dominated by an Active Galactic Nucleus, both globally as w
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::e40e294cfe1a75cdfe6788d69366edd6
http://hdl.handle.net/10261/141434
http://hdl.handle.net/10261/141434
CO in Hickson compact group galaxies with enhanced warm H 2 emission: Evidence for galaxy evolution?
Publikováno v:
Astronomy and Astrophysics
A24-177
A24-177
Context. Galaxies in Hickson Compact Groups (HCGs) are believed to experience morphological transformations from blue, star-forming galaxies to red, early-type galaxies. Galaxies with a high ratio between the luminosities of the warm H2 to the 7.7 μ
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______3158::00524c16aad28794eb53600937013e65
http://hdl.handle.net/11427/35104
http://hdl.handle.net/11427/35104
Galaxies in Hickson Compact Groups (HCGs) are believed to experience morphological transformations from blue, star-forming galaxies to red, early-type galaxies. Galaxies with a high ratio between the luminosities of the warm H2 to the 7.7mu PAH emiss
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cfde92143965f5ef2eff66d82a14cc9f
Context. High-resolution data from Spitzer, Herschel, and Planck allow us to probe the entire spectral energy distribution (SED) of morphologically separated components of the dust emission from nearby galaxies and allow a more detailed comparison be
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=core_ac_uk__::8994e10b9e5ac799acbb4e267e066368
https://clok.uclan.ac.uk/10941/1/10941_popescu.pdf
https://clok.uclan.ac.uk/10941/1/10941_popescu.pdf
Autor:
Natale, G., Tuffs, R. J., Xu, C. K., Popescu, C. C., Fischera, J., Lisenfeld, U., Lu, N., Appleton, P., Dopita, M., Duc, P. -A, Gao, Y., William Reach, Sulentic, J., Yun, M.
Publikováno v:
Galaxy Mergers in an evolving Universe: Astronomical Society of the Pacific Conference Series
NASA Astrophysics Data System
Digibug. Repositorio Institucional de la Universidad de Granada
instname
NASA Astrophysics Data System
Digibug. Repositorio Institucional de la Universidad de Granada
instname
We investigated the star formation efficiency for all the dust emitting sources in Stephan's Quintet (SQ). We inferred star formation rates using Spitzer MIR/FIR and GALEX FUV data and combined them with gas column density measurements by various aut
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::be9d5afd069305f42d6be783d74a207f
http://arxiv.org/abs/1203.3436
http://arxiv.org/abs/1203.3436
Autor:
Verley, S., Leon, S., Verdes-Montenegro, L., Combes, F., Jose Sabater, Sulentic, J., Bergond, G., Espada, D., Lisenfeld, U., Odewahn, S. C.
Publikováno v:
Digibug. Repositorio Institucional de la Universidad de Granada
instname
NASA Astrophysics Data System
instname
NASA Astrophysics Data System
The role of the environment on galaxy evolution is still not fully understood. In order to quantify and set limits on the role of nurture one must identify and study a sample of isolated galaxies. The AMIGA project "Analysis of the Interstellar Mediu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d241c69b084804d3b9005911e687ebe3
http://hdl.handle.net/10481/28390
http://hdl.handle.net/10481/28390
Publikováno v:
Digibug. Repositorio Institucional de la Universidad de Granada
instname
instname
International conference “Galaxies in Isolation: Exploring Nature vs. Nurture” held in Granada (Spain), May 12–15, 2009.
The project AMIGA (Analysis of the interstellar Medium of Isolated GAlaxies) provides a statistically significant samp
The project AMIGA (Analysis of the interstellar Medium of Isolated GAlaxies) provides a statistically significant samp
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bad6b198d6ab2b0036afd4c67dd886f1
http://hdl.handle.net/10481/28388
http://hdl.handle.net/10481/28388
Publikováno v:
Proceedings of the International Astronomical Union 2, IAU Symposium #237
Triggered Star Formation in a Turbulent ISM, International Astronomical Union. Symposium no. 237, held 14-18 August, 2006 in Prague, Czech Republic, S237, #86
Triggered Star Formation in a Turbulent ISM, International Astronomical Union. Symposium no. 237, held 14-18 August, 2006 in Prague, Czech Republic, S237, #86, 2007, Prague, Czech Republic. pp.398
Triggered Star Formation in a Turbulent ISM, International Astronomical Union. Symposium no. 237, held 14-18 August, 2006 in Prague, Czech Republic, S237, #86
Triggered Star Formation in a Turbulent ISM, International Astronomical Union. Symposium no. 237, held 14-18 August, 2006 in Prague, Czech Republic, S237, #86, 2007, Prague, Czech Republic. pp.398
I will present a project aimed at characterizing systematically the intergalactic star formation taking place in gas expelled from galaxies into the IGM by tidal forces during close encounters. A part of the ejected gas collapses to form new stars an
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::561a71bdd479448f8b6cbe19696f1682
https://hal.archives-ouvertes.fr/hal-00129614
https://hal.archives-ouvertes.fr/hal-00129614