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相关论文: Circumnuclear star-forming regions in early type s…

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(Abridged) Gas and star velocity dispersions have been derived for four circumnuclear star-forming regions (CNSFRs) and the nucleus of the spiral galaxy NGC2903 using high resolution spectroscopy in the blue and far red. Stellar velocity…

星系天体物理 · 物理学 2015-05-13 Guillermo F. Hagele , Angeles I. Diaz , Monica V. Cardaci , Elena Terlevich , Roberto Terlevich

(Abbr.) We present high resolution (R~20000) spectra in the blue and the far red of cicumnuclear star-forming regions (CNSFRs) in three early type spirals (NGC3351, NGC2903 and NGC3310) which have allowed the study of the kinematics of…

We have measured gas and stellar velocity dispersions in 5 circumnuclear starforming regions (CNSFRs) and the nucleus of the barred spiral galaxy NGC 3351. The stellar dispersions have been obtained from high resolution spectra of the CaT…

Gas and star velocity dispersions have been derived for eight circumnuclear star-forming regions (CNSFRs) and the nucleus of the spiral galaxy NGC3310 using high resolution spectroscopy in the blue and far red. Stellar velocity dispersions…

宇宙学与河外天体物理 · 物理学 2015-05-14 Guillermo F. Hagele , Angeles I. Diaz , Monica V. Cardaci , Elena Terlevich , Roberto Terlevich

(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

[Abbreviated] We review the results of high dispersion spectroscopy of 17 circumnuclear starforming regions (CNSFRs) in 3 nearby early spiral galaxies, NGC2903, NGC3310 and NGC3351. We find that single Gaussian fitting to the H$\beta$ and…

宇宙学与河外天体物理 · 物理学 2016-11-26 Guillermo F. Hagele , Angeles I. Diaz , Roberto Terlevich , Elena Terlevich , Guillermo L. Bosch , Monica V. Cardaci

In this third paper of a series, we study the kinematics of the ionised gas and stars, calculating the dynamical masses of the circumnuclear star-forming regions in the ring of of the face-on spiral NGC 7742. We have used high spectral…

星系天体物理 · 物理学 2025-04-02 S. Zamora , A. I. Díaz , Roberto Terlevich , Elena Terlevich , R. Amorín

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 analyze the kinematics of the central regions of five isolated Seyfert spiral galaxies from the DEGAS sample (four with new data presented in this paper, IC184, UGC3223, NGC2639, NGC6814, and NGC6951 from our previous data), by using…

天体物理学 · 物理学 2009-11-10 I. Marquez , J. Masegosa , F. Durret , R. M. Gonzalez Delgado , M. Moles , J. Maza , E. Perez , M. Roth

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

The study of stellar kinematic properties may provide hints on the formation and evolution of elliptical and lenticular galaxies. Although most previous studies have focused on the large scale of these galaxies, their central regions…

星系天体物理 · 物理学 2016-10-06 T. V. Ricci , J. E. Steiner , R. B. Menezes

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

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

In recent years, Circumnuclear Star Forming Regions (CNSFRs) have been studied in different frequencies and telescopes, diverse studies about connection between nuclear activity and star formation in the CNSFRs were doing using optical…

星系天体物理 · 物理学 2018-01-26 I. Villicaña-Pedraza , D. Mast , A. Díaz , F. Carreto-Parra , G. Hagele , M. Cardaci

High-resolution observations of ionized and molecular gas in the nuclear regions of galaxies are indispensable for delineating the interplay of star formation, gaseous inflows, stellar radiation, and feedback processes. Combining our new…

星系天体物理 · 物理学 2021-06-23 Yulong Gao , Fumi Egusa , Guilin Liu , Kotaro Kohno , Min Bao , Kana Morokuma-matsui , Xu Kong , Xiaoyang Chen

The formation process of high-mass stars (>8M$_\odot$) is poorly constrained, particularly, the effects of clump fragmentation creating multiple systems and the mechanism of mass accretion onto the cores. We study the fragmentation of dense…

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

The initial velocity dispersion of newborn stars is a major unconstrained aspect of star formation theory. Using near-infrared spectra obtained with the APOGEE spectrograph, we show that the velocity dispersion of young (1-2 Myr) stars in…

In the framework of understanding the gas and stellar kinematics and their relations to AGNs and galaxy evolution scenarios, we present spatially resolved distributions and kinematics of the stars and gas in the central $\sim 800$-pc radius…

We present new maps of emission-line flux distributions and kinematics in both ionized (traced by HI and [FeII] lines) and molecular (H2) gas of the inner 0.7x0.7kpc2 of the galaxy NGC4303, with a spatial resolution 40-80pc and velocity…

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