FISICA observations of the starburst galaxy, NGC 1569

2006 ◽  
Vol 50 (4-5) ◽  
pp. 433-435
Author(s):  
D.M. Clark ◽  
S.S. Eikenberry ◽  
S.N. Raines ◽  
N. Gruel ◽  
R. Elston ◽  
...  
Keyword(s):  
Starburst Galaxy ◽  
Ngc 1569

The Environment of X-Ray Binaries in the Dwarf Starburst Galaxy NGC 1569

2008 ◽  
Author(s):  
David M. Clark ◽  
Stephen S. Eikenberry ◽  
Steven N. Raines ◽  
Reba M. Bandyopadhyay ◽  
Stefanie Wachter ◽  
...  
Keyword(s):  
Starburst Galaxy ◽  
X Ray ◽  
X Ray Binaries ◽  
Ngc 1569

scholarly journals The chaotic ISM of the post(?)-starburst galaxy NGC 1569

2003 ◽  
Vol 212 ◽  
pp. 549-550
Author(s):  
Reginald J. Dufour ◽  
Brent A. Buckalew ◽  
Patrick L. Shopbell ◽  
Donald K. Walter
Keyword(s):  
Supernova Remnants ◽  
Large Scale ◽  
Wide Band ◽  
Primary Data ◽  
Starburst Galaxy ◽  
Main Body ◽  
Ionized Gas ◽  
Super Star Clusters ◽  
Dust Distribution ◽  
Ngc 1569

We present the results and analysis of HST-wfpc2 imagery of the starburst galaxy NGC 1569 (d = 2.2 Mpc), which permit unprecedented resolution (~ 1pc) of the ionized gas and stellar population. The primary data in our analysis consists of images taken through narrow-band filters isolating Hβ, Hα, [O iii]λ5007, and [S ii]λλ6717+30, as part of go Program 8133. A variety of color-coded and grey-scaled maps of the morphology, ionization structure, and dust distribution are presented. Unsharp masks of the Hα images show a very chaotic structure for the ionized gas, with numerous filaments and arc-like bright rim features across the entire galaxy, but without significant large-scale ionization variations. Variations in the ionization and line-of-sight reddening occur on smaller scales (~ 10 – 50 pc), with numerous low-ionization semi-stellar knots seen throughout the main body of the galaxy, even within the ‘hole’ in the ionized gas distribution around the central super star clusters previously noted from H i maps. Several of these features have strong [S ii] emission indicative of being supernova remnants. We combine these data with archival wide-band HST-wfpc2 imagery to quantitatively evaluate the source(s) of the (largely photo-) ionized gas.

scholarly journals Star cluster formation and evolution in the dwarf starburst galaxy NGC 1569

2004 ◽  
Vol 347 (1) ◽  
pp. 17-28 ◽  
Author(s):  
P. Anders ◽  
R. de Grijs ◽  
U. Fritze-v. Alvensleben ◽  
N. Bissantz
Keyword(s):  
Cluster Formation ◽  
Star Cluster ◽  
Starburst Galaxy ◽  
Formation And Evolution ◽  
Ngc 1569

scholarly journals GROUND-BASED NEAR-INFRARED CENSUS FOR YOUNG STAR CLUSTERS IN THE DWARF STARBURST GALAXY NGC 1569

2010 ◽  
Vol 43 (1) ◽  
pp. 1-8 ◽  
Author(s):  
Jae-Mann Kyeong ◽  
Eon-Chang Sung ◽  
Sang-Chul Kim ◽  
Brian Chaboyer
Keyword(s):  
Near Infrared ◽  
Star Clusters ◽  
Young Star ◽  
Starburst Galaxy ◽  
Young Star Clusters ◽  
Ngc 1569

Discovery of a Double Circumnuclear Ring and Minibar in the Starburst Galaxy M83

1998 ◽  
Vol 116 (6) ◽  
pp. 2834-2840 ◽  
Author(s):  
Debra Meloy Elmegreen ◽  
Frederick R. Chromey ◽  
Aaron R. Warren
Keyword(s):  
Starburst Galaxy

scholarly journals The Discovery of Spiral Arms in the Starburst Galaxy M82

2005 ◽  
Vol 628 (1) ◽  
pp. L33-L36 ◽  
Author(s):  
Y. D. Mayya ◽  
L. Carrasco ◽  
A. Luna
Keyword(s):  
Starburst Galaxy ◽  
Spiral Arms

scholarly journals OH main line masers in the M 82 starburst

2007 ◽  
Vol 3 (S242) ◽  
pp. 427-431
Author(s):  
M. K. Argo ◽  
A. Pedlar ◽  
T. W. B. Muxlow ◽  
R. J. Beswick
Keyword(s):  
Central Region ◽  
Supernova Remnants ◽  
Main Line ◽  
Line Of Sight ◽  
Starburst Galaxy ◽  
Large Array ◽  
Satellite Line ◽  
Very Large Array

AbstractA study of the distribution of OH gas in the central region of the nearby active starburst galaxy M82 has confirmed two previously known bright masers and revealed several new main line masers. Three of these are seen only at 1665 MHz, one is detected only at 1667 MHz, while the rest are detected in both lines. Observations covering both the 1665 and 1667 MHz lines, conducted with both the Very Large Array (VLA) and the Multi-Element Radio Linked Interferometer Network (MERLIN), have been used to accurately measure the positions and velocities of these features. This has allowed a comparison with catalogued continuum features in the starburst such as HII regions and supernova remnants, as well as known water and satellite line OH masers. Most of the main line masers appear to be associated with known HII regions although the two detected only at 1665 MHz are seen along the same line of sight as known supernova remnants.

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