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相关论文: Stellar Populations in Circumnuclear Star Forming …

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We present a study of the stellar populations and gas physical conditions in Circumnuclear Star Forming Regions (CNSFRs) based on spectrophotometric data, including the 7000 angstroms to 1 micron spectral range, which is of great interest…

天体物理学 · 物理学 2007-05-23 Enrique Perez-Montero , Angeles I. Diaz , Marcelo Castellanos

We present a spectrophotometric study of circumnuclear star forming regions (CNSFR) in the early type spiral galaxies: NGC 2903, NGC 3351 and NGC 3504, all of them of over solar metallicity according to standard empirical calibrations. A…

天体物理学 · 物理学 2007-05-23 A. I. Diaz , E. Terlevich , M. Castellanos , G. F. Hagele

Circumnuclear star forming regions (CNSFR) are massive clusters found close to galactic nuclei. These entities give us an excellent opportunity to study star formation in environments with high metallicity and to relate it with active…

星系天体物理 · 物理学 2025-04-02 S. Zamora , Ángeles I. Díaz

We present the results of a study of young unresolved stellar groupings (clusters, OB associations, and their complexes) associated with HII regions, based on the coupling of spectroscopic, photometric and H{\alpha} spectrophotometric…

星系天体物理 · 物理学 2023-07-13 A. S. Gusev , F. Sakhibov , O. V. Egorov , V. S. Kostiuk , E. V. Shimanovskaya

(Abbr.) A study of cicumnuclear star-forming regions (CNSFRs) in several early type spirals has been made in order to investigate their main properties: stellar and gas kinematics, dynamical masses, ionising stellar masses, chemical…

天体物理学 · 物理学 2009-12-04 Angeles I. Diaz , Guillermo F. Hagele , Elena Terlevich , Roberto Terlevich

Preliminary results from spectrophotometric observations of Circumnuclear Star Forming Regions (CNSFRs) in the spiral galaxies NGC 2903, NGC 3351 and NGC 3504 are presented. The analysis is focused both on the determination of elemental…

天体物理学 · 物理学 2007-05-23 M. Castellanos , A. I. Diaz , M. Alvarez-Alvarez , E. Terlevich

We present photometry in U, B, V, R and I continuum bands and in H$\alpha$ and H$\beta$ emission lines for a sample of 336 circumnuclear star forming regions (CNSFR) located in early type spiral galaxies with different levels of activity in…

星系天体物理 · 物理学 2017-01-04 Mar Álvarez-Álvarez , Angeles I. Díaz , Elena Terlevich , Roberto Terlevich

This work aims to derive the physical properties of the CNSFRs in the ring of the face-on spiral NGC 7742 using IFS observations. We have selected 88 individual ionising clusters that power HII regions populating the ring of the galaxy that…

星系天体物理 · 物理学 2023-07-19 S. Zamora , A. I. Díaz

V,R,I continuum bands and Halpha + [NII] photometry for circumnuclear star forming regions (CNSFR) is presented, for galaxies with different kinds of nuclear activity: NGC 7469 (Sy 1), NGC 1068 (Sy 2), NGC 7177 (LINER) and NGC 3310…

Results of a study of physical parameters of stellar population in star formation regions in galaxies with signs of peculiarity NGC 3963 and NGC 7292 are presented. The study was carried out based on the analysis of photometric (UBVRI…

星系天体物理 · 物理学 2024-10-10 A. S. Gusev , F. Kh. Sakhibov , A. V. Moiseev , V. S. Kostiuk , D. V. Oparin

We present high-resolution near-infrared imaging obtained using adaptive optics and HST/NICMOS, and ground-based spectroscopy of the hot-spot galaxy NGC2903. Our near-infrared resolution imaging enables us to resolve the infrared hot spots…

天体物理学 · 物理学 2009-10-31 A. Alonso-Herrero , S. D. Ryder , J. H. Knapen

Circumnuclear star forming regions, also called hotspots, are often found in the inner regions of some spiral galaxies where intense processes of star formation are taking place. In the UV, massive stars dominate the observed circumnuclear…

天体物理学 · 物理学 2008-01-22 Angeles I. Diaz , Elena Terlevich , Guillermo F. Hagele , Marcelo Castellanos

The circumnuclear star-forming ring of the barred spiral galaxy NGC 1097 provides a unique laboratory to study star formation under extreme conditions. This work aims to derive the physical properties of the circumnuclear star-forming…

星系天体物理 · 物理学 2026-02-11 Sandra Zamora , Angeles I. Díaz , Asier Castrillo

We present Hubble Space Telescope blue spectra at intermediate spectral resolution for the nuclei of 23 nearby disk galaxies. These objects were selected to have nebular emission in their nuclei, and span a range of emission-line…

Recent observations supported by theoretical models have lead to the view that giant and supergiant stars are over abundant, and/or a high metallicity component may be present, in the stellar populations at the centres of active galaxies.…

天体物理学 · 物理学 2009-10-30 M. Serote Roos , C. Boisson , M. Joly , M. J. Ward

We present a study of the stellar populations of a sample of 39 local, field early-type galaxies whose HI properties are known from interferometric data. Our aim is to understand whether stellar age and chemical composition depend on the HI…

天体物理学 · 物理学 2009-11-13 Paolo Serra , Scott C. Trager , Tom A. Oosterloo , Raffaella Morganti

We investigate the stellar populations in the star forming ring of the luminous infrared galaxy NGC 7469. We use Hubble Space Telescope multi-wavelength (UV through NIR) imaging complemented with new K-band ground-based long-slit…

天体物理学 · 物理学 2011-02-11 Tanio Diaz-Santos , Almudena Alonso-Herrero , Luis Colina , Stuart D. Ryder , Johan H. Knapen

We have obtained long-slit observations in the optical and near infrared of 12 circumnuclear HII regions (CNSFR) in the early type spiral galaxies NGC 2903, NGC 3351 and NGC 3504 with the aim of deriving their chemical abundances. Only for…

天体物理学 · 物理学 2009-11-13 Angeles I. Diaz , Elena Terlevich , Marcelo Castellanos , Guillermo F. Hagele

A stellar population synthesis model, suitable for comparison with Giant Extragalactic HII Regions (GEHRs), is constructed incorporating the recent developments in modelling stellar evolution by Maeder and co-workers and stellar atmospheres…

天体物理学 · 物理学 2016-08-30 Y. D. Mayya

The majority of spiral and elliptical galaxies in the Universe host very dense and compact stellar systems at their centres known as nuclear star clusters (NSCs). In this work we study the stellar populations and star formation histories…

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