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Sánchez Menguiano, L
126  Ergebnisse:
Personensuche X
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1

The CAVITY project: The spatially resolved stellar populati..:

Conrado, Ana M. ; González Delgado, Rosa M. ; García-Benito, Rubén...
Astronomy & Astrophysics.  687 (2024)  - p. A98 , 2024
Link: https://doi.org/10.1051/..
 
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2

More fundamental than the fundamental metallicity relation:..:

Sánchez-Menguiano, Laura ; Sánchez, Sebastián F. ; Sánchez Almeida, Jorge.
Astronomy & Astrophysics.  682 (2024)  - p. L11 , 2024
Link: https://doi.org/10.1051/..
 
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3

Stellar mass is not the best predictor of galaxy metallicit..:

Sánchez-Menguiano, Laura ; Sánchez Almeida, Jorge ; Sánchez, Sebastián F..
Astronomy & Astrophysics.  681 (2024)  - p. A121 , 2024
Link: https://doi.org/10.1051/..
 
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4

Stellar mass-metallicity relation throughout the large-scal..:

Domínguez-Gómez, Jesús ; Pérez, Isabel ; Ruiz-Lara, Tomás...
Astronomy & Astrophysics.  680 (2023)  - p. A111 , 2023
Link: https://doi.org/10.1051/..
 
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5

Galaxies in voids assemble their stars slowly:

Domínguez-Gómez, Jesús ; Pérez, Isabel ; Ruiz-Lara, Tomás...
Nature.  619 (2023)  7969 - p. 269-271 , 2023
Link: https://doi.org/10.1038/..
 
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6

Arm–interarm gas abundance variations explored with MUSE: t..:

Sánchez-Menguiano, Laura ; Sánchez, Sebastián F ; Pérez, Isabel...
Monthly Notices of the Royal Astronomical Society.  492 (2020)  3 - p. 4149-4163 , 2020
Link: https://doi.org/10.1093/..
 
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7

Oxygen abundance profiles with MUSE: Radial gradients and w..:

Sánchez-Menguiano, Laura ; Sánchez, Sebastián F. ; Pérez, Isabel
Proceedings of the International Astronomical Union.  14 (2018)  A30 - p. 260-260 , 2018
Link: https://doi.org/10.1017/..
 
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8

Two-dimensional multi-component photometric decomposition o..:

Méndez Abreu, J ; Ruiz Lara, T ; Sánchez Menguiano, L...
info:eu-repo/semantics/altIdentifier/wos/WOS:000394465000032.  , 2017
Link: http://hdl.handle.net/11..
 
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9

No direct coupling between bending of galaxy disc stellar a..:

Ruiz-Lara, Tomás ; Pérez, Isabel ; Florido, Estrella...
Proceedings of the International Astronomical Union.  11 (2016)  S321 - p. 278-278 , 2016
Link: https://doi.org/10.1017/..
 
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10

Shape of the oxygen abundance profiles in CALIFA face-on sp..:

Sánchez Menguiano, L ; Sánchez, S. F ; Pérez, I...
A&A 587, A70 (2016).  , 2016
Link: https://doi.org/10.1051/..
 
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11

Pipe3D, a pipeline to analyse integral field spectroscopy d..:

Sánchez, S. F ; Pérez, E ; Sánchez Blázquez, P...
Revista Mexicana de Astronomía y Astrofísica Volumen: 52 Número: 1 Páginas: 171-220.  , 2016
Link: http://repositorio.uchil..
 
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12

No direct coupling between bending of galaxy disc stellar a..:

Ruiz Lara, T ; Pérez, I ; Florido, E...
MNRAS 456, L35–L39 (2016).  , 2016
Link: https://doi.org/10.1093/..
 
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13

The CALIFA Survey: Exploring the Oxygen Abundance in the Lo..:

Sánchez, Sebastian ; Sánchez-Menguiano, Laura ; Marino, Raffaella...
Galaxies.  3 (2015)  4 - p. 164-183 , 2015
Link: https://doi.org/10.3390/..
 
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14

Imprints of galaxy evolution on H II regions: memory of the..:

Sánchez, S. F ; Pérez, E ; Rosales Ortega, F. F...
ICTS-2009-10.  , 2015
Link: https://hdl.handle.net/2..
 
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15

Census of HII regions in NGC 6754 derived with MUSE: Constr..:

Sánchez, S ; Galbany, Lluis ; Pérez, E...
Astronomy & Astrophysics Volumen: 573 Número de artículo: A105.  , 2015
Link: https://doi.org/10.1051/..
 
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