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1
Star formation in HI tails HCG 92, HCG 100 and six interacting systems
Star formation in HI tails HCG 92, HCG 100 and six interacting systems
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Star formation in HI tails HCG 92, HCG 100 and six interacting systems

D. F. de Mello F Urrutia-Viscarra; Cláudia Lúcia Mendes de Oliveira; S Torres-Flores; E. R Carrasco; Eduardo Serra Cypriano

Monthly Notices of the Royal Astronomical Society Oxford v. 426, p. 2441-2450, 2012

Oxford 2012

Item não circula. Consulte sua biblioteca.(Acessar)

2
Probing the nature of the pre-merging system Hickson Compact Group 31 through integral field unit data
Probing the nature of the pre-merging system Hickson Compact Group 31 through integral field unit data
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Probing the nature of the pre-merging system Hickson Compact Group 31 through integral field unit data

M Alfaro-Cuello S Torres-Flores; E. R Carrasco; Cláudia Mendes de Oliveira; D. F de Mello; P Amram

Monthly Notices of the Royal Astronomical Society Oxford v. 453, p.1355–1370, 2015

Oxford 2015

Item não circula. Consulte sua biblioteca.(Acessar)

3
The miniJPAS survey Identification and characterization of the emission line galaxies down to z < 0.35 in the AEGIS field
The miniJPAS survey Identification and characterization of the emission line galaxies down to z < 0.35 in the AEGIS field
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The miniJPAS survey Identification and characterization of the emission line galaxies down to z < 0.35 in the AEGIS field

G. Martínez-Solaeche L. Raul Abramo; L Sodré Jr.; A Ederoclite; C. Mendes de Oliveira

Astronomy & Astrophysics Les Ulis: EDP Sciences, 2022 v. 661, 21p., 9 de maio de 2022, número do artigo: A99

Les Ulis 2022

Item não circula. Consulte sua biblioteca.(Acessar)

4
The miniJPAS survey: White dwarf science with 56 optical filters
The miniJPAS survey: White dwarf science with 56 optical filters
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The miniJPAS survey: White dwarf science with 56 optical filters

C López-Sanjuan Luis Raul Weber Abramo; Laerte Sodré Júnior; Claudia Lucia Mendes de Oliveira

Astronomy & Astrophysics Les Ulis: EDP Sciences, 2022 v. 665, A151, 2022

Les Ulis EDP Sciences 2022

Item não circula. Consulte sua biblioteca.(Acessar)

5
Star-forming regions and the metallicity gradients in the tidal tails the case of NGC 92
Star-forming regions and the metallicity gradients in the tidal tails the case of NGC 92
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Star-forming regions and the metallicity gradients in the tidal tails the case of NGC 92

S Torres-Flores S Scarano Júnior; Cláudia Lúcia Mendes de Oliveira; D. F. de Mello; P Amram; H Plana

Monthly Notices of the Royal Astronomical Society Oxford v. 438, p. 1894\20131908, 2014

Oxford 2014

Item não circula. Consulte sua biblioteca.(Acessar)

6
Star formation activity and gas stripping in the Cluster Projected Phase-Space (CPPS)
Star formation activity and gas stripping in the Cluster Projected Phase-Space (CPPS)
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Star formation activity and gas stripping in the Cluster Projected Phase-Space (CPPS)

Jonathan D. Hernández-Fernández C. P Haines; A Diaferio; J Iglesias-Páramo; Cláudia Lúcia Mendes de Oliveira; J. M Vilchez

Monthly Notices of the Royal Astronomical Society Oxford v. 438, p. 2186\20132200, 2014

Oxford 2014

Item não circula. Consulte sua biblioteca.(Acessar)

7
The connection between the origins of globular clusters (GCs) and the evolution of their host galaxy
The connection between the origins of globular clusters (GCs) and the evolution of their host galaxy
Material Type:
Artigo de Congresso 		Adicionar ao Meu Espaço

The connection between the origins of globular clusters (GCs) and the evolution of their host galaxy

A Cortesi Claudia Lucia Mendes de Oliveira; A Chies-Santos; S Bamford; M Merrifield; A Romanowsky; J Arnold; V Pota; D Forbes; L Coccato; J Brodie; C Usher; J Strader; C Foster; Latin American Regional IAU Meeting (14. 2013 Florianópolis, Brazil)

Revista Mexicana de Astronomía y Astrofísica. Serie de Conferencias México v. 44, p. 174, 2014

México 2014

Item não circula. Consulte sua biblioteca.(Acessar)

8
Observations of the first electromagnetic counterpart to a gravitational-wave source by the TOROS collaboration
Observations of the first electromagnetic counterpart to a gravitational-wave source by the TOROS collaboration
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Observations of the first electromagnetic counterpart to a gravitational-wave source by the TOROS collaboration

M C Díaz L M Macri; D Garcia Lambas; C Mendes de Oliveira; J L Nilo Castellón; T Ribeiro; B Sánchez; W Schoenell; Luis Raul Weber Abramo; S Akras; J S Alcaniz; R Artola; M Beroiz; S Bonoli; J Cabral; R Camuccio Castillo. M; V Chavushyan; P Coelho; C Colazo; M V Costa Duarte; H Cuevas Larenas; D L DePoy; M Domínguez Romero; D Dultzin; D Fernández; J García; C Girardini; D R Gonçalves; T S Gonçalves; S Gurovich; V Jiménez-Teja; A Kanaan; M Lares R. Lopes de Oliveira7,16,; O López-Cruz; J L Marshall; R Melia; A Molino; N Padilla; T Peñuela; V M Placco; C Quiñones; A Ramírez Rivera; V Renzi; L Riguccini; E Ríos-López; H Rodriguez; L Sampedro; M Schneiter; L Sodré; M Starck; S Torres-Flores; M Tornatore; A Zadrożny

The Astrophysical Journal Letters Bristol v. 848, n. 2 , p. L29/1-L29/5, 2017

Bristol 2017

Item não circula. Consulte sua biblioteca.(Acessar)

9
Metallicity gradients and newly created star-forming systems in interacting galaxies
Metallicity gradients and newly created star-forming systems in interacting galaxies
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Metallicity gradients and newly created star-forming systems in interacting galaxies

Cláudia Lúcia Mendes de Oliveira IAU General Assembly (29. 2015 Honolulu, USA)

Meeting Abstracts Paris: International Astronomical Union, 2015

Paris International Astronomical Union 2015

Item não circula. Consulte sua biblioteca.(Acessar)

10
An analysis of the composite stellar population in M32
An analysis of the composite stellar population in M32
Material Type:
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An analysis of the composite stellar population in M32

P Coelho Cláudia Lúcia Mendes de Oliveira; R. Cid Fernandes; IAU Symposium (262. 2009 Rio de Janeiro, RJ, Brazil)

Stellar populations : planning for the next decade. Proceedings Cambridge : Cambridge University Press, 2010

Cambridge Cambridge University Press 2010

Item não circula. Consulte sua biblioteca.(Acessar)

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