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相关论文: The Star Formation History of the Blue Compact Dwa…

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We present HST/WFPC2 single-star photometry for the blue dwarf galaxy UGCA 290, whose morphology is intermediate between classic iE Blue Compact Dwarfs and blue dwarfs which exhibit no red background sheet of older stars. The…

天体物理学 · 物理学 2009-10-31 Mary M. Crone , Regina E. Schulte-Ladbeck , Ulrich Hopp , Laura Greggio

We present a quantitative star formation history of the nearby dwarf galaxy UGCA 92. This irregular dwarf is situated in the vicinity of the Local Group of galaxies in a zone of strong Galactic extinction (IC 342 group of galaxies). The…

宇宙学与河外天体物理 · 物理学 2015-06-04 Lidia Makarova , Dmitry Makarov , Sergey Savchenko

The recent history of star formation in the BCD galaxy VII Zw403, is analysed with accounts for the dynamics of the remnant generated either by an instantaneous burst or by a continuous star formation event. We have re-observed VII Zw403…

天体物理学 · 物理学 2009-11-07 S. Silich , G. Tenorio-Tagle , C. Munoz-Tunon , L. M. Cairos

We determine and examine the star-formation rates of 50 well known, local Blue Compact Dwarf (BCD) galaxies based on their 1.4 GHz and 60 $\mu$m luminosities. We find that in cases for which both radio and far-infrared luminosities are…

天体物理学 · 物理学 2008-12-18 A. M. Hopkins , R. E. Schulte-Ladbeck , I. O. Drozdovsky

(Abridged) Low-luminosity, active star-forming blue compact galaxies (BCGs) are excellent laboratories for investigating the process of star formation on galactic scales and probing the interplay between massive stars and the surrounding…

星系天体物理 · 物理学 2020-02-19 L. M. Cairós , J. N. González-Pérez

We study the stellar populations, star formation histories and star formation properties for a sample of blue compact dwarf galaxies (BCDs) selected by cross-correlating the Gil de Paz et al. (2003) sample with the Sloan Digital Sky Survey…

宇宙学与河外天体物理 · 物理学 2015-03-17 Yinghe Zhao , Qiusheng Gu , Yu Gao

We have derived the star formation history (SFH) of the blue compact dwarf galaxy IZw18 through comparison of deep HST/ACS data with synthetic color magnitude diagrams. A statistical analysis was implemented for the identification of the…

宇宙学与河外天体物理 · 物理学 2015-06-15 F. Annibali , M. Cignoni , M. Tosi , R. P. van der Marel , A. Aloisi , G. Clementini , R. Contreras Ramos , G. Fiorentino , M. Marconi , I. Musella

We present evidence for the existence of an old stellar halo in the Blue Compact Dwarf galaxy VII Zw 403. VII Zw 403 is the first Blue Compact Dwarf galaxy for which a clear spatial segregation of the resolved stellar content into a…

天体物理学 · 物理学 2009-10-31 Regina E. Schulte-Ladbeck , Ulrich Hopp , Mary M. Crone , Laura Greggio

We infer the star formation history in different regions of the blue compact dwarf NGC 1705 by comparing synthetic color-magnitude diagrams with HST optical and near-infrared photometry. We find that NGC 1705 is not a young galaxy because…

天体物理学 · 物理学 2009-11-10 F. Annibali , L. Greggio , M. Tosi , A. Aloisi , C. Leitherer

It has long been speculated that Blue Compact Dwarf galaxies (BCDs) are formed through the interaction between low-mass gas-rich galaxies, but a few candidates of such systems have been studied in detail. We study a sample of compact…

星系天体物理 · 物理学 2022-12-15 Daya Nidhi Chhatkuli , Sanjaya Paudel , Rajesh Kumar Bachchan , Binil Aryal , Jaewon Yoo

We present resolved-star VI photometry of the Local Group dwarf irregular galaxy IC1613 reaching I~23.5, obtained with the wide-field camera at the 2.5m Isaac Newton Telescope. A fit to the stellar density distribution shows an exponential…

We report H$\alpha$ observations of a sample of very isolated blue compact galaxies (BCGs) located in the direction of large cosmic voids obtained to understand their stellar population compositions, the present star formation (SF)…

宇宙学与河外天体物理 · 物理学 2013-07-09 Adi Zitrin , Noah Brosch , Benny Bilenko

Two blue compact dwarf galaxies Mkn 104 and I Zw 97 are studied photometrically and spectroscopically. Mkn 104 is found to contain three distinct bright star forming regions, whereas I Zw 97 is found to contain three bright and two faint…

宇宙学与河外天体物理 · 物理学 2015-05-13 S Ramya , D K Sahu , T P Prabhu

UGC 4483 is a nearby Blue Compact Dwarf (BCD) galaxy. HST observations have resolved the galaxy into single stars and this has led to the derivation of its star formation history and to a direct estimate of its stellar mass. We have…

宇宙学与河外天体物理 · 物理学 2015-06-05 Federico Lelli , Marc Verheijen , Filippo Fraternali , Renzo Sancisi

UGCA 320 is a gas-rich dwarf irregular galaxy which belongs to a nearby, relatively isolated group of dwarf galaxies. Here, we combine multi-band HST imaging data with deep long-slit SALT/RSS and integral-field VLT/MUSE spectral data to…

星系天体物理 · 物理学 2025-09-25 Adebusola B. Alabi , S. Ilani Loubser , Moses K. Mogotsi , N. Zabel

Images of five fields in the Local Group dwarf irregular galaxy NGC 6822 obtained with the {\it Hubble Space Telescope} in the F555W and F814W filters are presented. Photometry for the stars in these images was extracted using the…

天体物理学 · 物理学 2009-11-07 Ted K. Wyder

Crucial to a quantitative understanding of galaxy evolution are the properties of the inter-stellar medium that regulate galactic-scale star formation activity. We present here the results of a suite of star formation models applied to the…

宇宙学与河外天体物理 · 物理学 2015-05-30 E C Elson , W J G de Blok , R C Kraan-Korteweg

We present optical (UBVJ), ultraviolet (FUV, NUV), and high resolution atomic hydrogen (HI) observations of the nearby blue compact dwarf (BCD), VII Zw 403. We find that VII Zw 403 has a relatively high HI mass-to-light ratio for a BCD. The…

We present a detailed study of the Magellanic irregular galaxy NGC 4449 based on both archival and new photometric data from the Legacy Extragalactic UV Survey, obtained with the Hubble Space Telescope Advanced Camera for Surveys and Wide…

We present new WFC3/UVIS observations of UGC 4483, the closest example of a metal-poor blue compact dwarf galaxy, with a metallicity of $Z \simeq 1/15\ Z_{\odot}$ and located at a distance of $D \simeq 3.4$ Mpc. The extremely high quality…

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