Zobrazeno 1 - 10
of 114
pro vyhledávání: '"Ute Lisenfeld"'
Autor:
Qingzheng Yu, Taotao Fang, Cong Kevin Xu, Shuai Feng, Siyi Feng, Yu Gao, Xue-Jian Jiang, Ute Lisenfeld
Publikováno v:
The Astrophysical Journal Supplement Series, Vol 273, Iss 1, p 2 (2024)
We present a study of the molecular gas in early-mid stage major mergers, with a sample of 43 major-merger galaxy pairs selected from the Mapping Nearby Galaxies at Apache Point Observatory survey and a control sample of 195 isolated galaxies selecte
Externí odkaz:
https://doaj.org/article/d3f985fc5a3e4653afe4007a68d0987c
Autor:
J. M. van der Hulst, Angel R. Lopez-Sanchez, Jesús Falcón-Barroso, Isabel Pérez, T. Ruiz-Lara, Kathryn Kreckel, S. Duarte Puertas, S. Verley, R. van de Weygaert, Ute Lisenfeld, J. Domínguez-Gómez, Reynier Peletier
Publikováno v:
Digibug. Repositorio Institucional de la Universidad de Granada
instname
Digital.CSIC. Repositorio Institucional del CSIC
Astronomy & astrophysics, 658:A124. EDP Sciences
instname
Digital.CSIC. Repositorio Institucional del CSIC
Astronomy & astrophysics, 658:A124. EDP Sciences
Acknowledgements. We appreciate the detailed and useful comments of the referee which helped to improve the clarity of the paper. We acknowledge support (proyect AYA2017-84897-P) from the Spanish Ministerio de Economía y Competitividad, from the Eur
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a51ad342d937b7e6b09fce8ed77c1b71
http://hdl.handle.net/10481/73071
http://hdl.handle.net/10481/73071
Autor:
Enrico M Di Teodoro, Lorenzo Posti, S Michael Fall, Patrick M Ogle, Thomas Jarrett, Philip N Appleton, Michelle E Cluver, Martha P Haynes, Ute Lisenfeld
We present new and archival atomic hydrogen (\hi) observations of \galnum\ of the most massive spiral galaxies in the local Universe ($M_\star>10^{11} \, \mathrm{M}_\odot$). From 3D kinematic modeling of the datacubes, we derive extended \hi\ rotatio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e3312cb916eccca1f145c7d4e541ecdf
Autor:
Simon Verley, Almudena Zurita, Lourdes Verdes-Montenegro, V. Martínez-Badenes, Isabel Pérez, J. Sabater, Ute Lisenfeld, Stephane Leon, Francoise Combes, S. Díaz-García, D. Espada
Publikováno v:
Digibug. Repositorio Institucional de la Universidad de Granada
instname
Digital.CSIC. Repositorio Institucional del CSIC
instname
Digital.CSIC. Repositorio Institucional del CSIC
We thank the anonymous referee for a constructive and detailed report. This project has received funding from the European Union's Horizon 2020 research and innovation programme under the Marie Sklodowska Curie grant agreement No 893673. We acknowled
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c48ac3fc2fe89561dffd4417ca64abfe
http://hdl.handle.net/10481/71541
http://hdl.handle.net/10481/71541
Autor:
Elizaveta Sazonova, Katherine Alatalo, Timothy M. Heckman, Lauranne Lanz, Kristina Nyland, Ute Lisenfeld, Gregory F. Snyder, K. Decker French, C. M. Urry, Kate Rowlands, Susana E. Deustua, Justin A. Otter, Yuanze Luo, Anne M. Medling, Andreea Petric
How do galaxies transform from blue, star-forming spirals to red, quiescent early-type galaxies? To answer this question, we analyzed a set of 26 gas-rich, shocked post-starburst galaxies with Hubble Space Telescope (HST) imaging in B, I, and H bands
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::beb1363f1439744a270ca9d0d36e1253
http://arxiv.org/abs/2105.09956
http://arxiv.org/abs/2105.09956
Autor:
Cinthya N. Herrera, Dario Colombo, Frank Bigiel, Annie Hughes, M. Querejeta, Andrew Rigby, Santiago García-Burillo, Eva Schinnerer, Sharon Meidt, Toby J. T. Moore, C. G. Mundell, Ute Lisenfeld, Federico Lelli, J. M. D. Kruijssen, Jérôme Pety
Publikováno v:
Digibug. Repositorio Institucional de la Universidad de Granada
instname
Digibug: Repositorio Institucional de la Universidad de Granada
Universidad de Granada (UGR)
Astronomy & Astrophysics
ASTRONOMY & ASTROPHYSICS
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 645, pp.A97. ⟨10.1051/0004-6361/202038955⟩
instname
Digibug: Repositorio Institucional de la Universidad de Granada
Universidad de Granada (UGR)
Astronomy & Astrophysics
ASTRONOMY & ASTROPHYSICS
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 645, pp.A97. ⟨10.1051/0004-6361/202038955⟩
Tidal dwarf galaxies (TDGs) are gravitationally bound condensations of gas and stars that 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
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d1e1f9abec06474891b451f305834d12
http://hdl.handle.net/10481/67199
http://hdl.handle.net/10481/67199
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
Context. Dust is formed out of stellar material and it is constantly affected by different mechanisms occurring in the interstellar medium. Depending on their size, the behaviour of dust grains vary under these mechanisms and, therefore, the dust gra
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5db3b84fe95baca9cf7abfdb8a780ae0
http://arxiv.org/abs/2002.01945
http://arxiv.org/abs/2002.01945
Publikováno v:
The Astrophysical Journal. 918:55
Previous studies have shown significant differences in the enhancement of the star-formation rate (SFR) and the star-formation efficiency (SFE=SFR/M_mol) between spiral-spiral and spiral-elliptical mergers. In order to shed light on the physical mech
We present CO observations of 78 spiral galaxies in local merger pairs. These galaxies representa subsample of a Ks-band selected sample consisting of 88 close major-merger pairs (HKPAIRs), 44 spiral-spiral (S+S) pairs and 44 spiral-elliptical (S+E)
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::852988cce4628564da17fa52a9ab522a
We present a study of the HI gas content of a large K-band selected sample of 88 close major-merger pairs of galaxies (H-KPAIR) which were observed by $\it Herschel$. We obtained the 21 cm HI fine-structure emission line data for a total of 70 pairs
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::68a43e01098883abbc377673038be889
http://arxiv.org/abs/1804.03500
http://arxiv.org/abs/1804.03500