HI Observations of the Irregular Galaxy IC 10

1983 ◽  
pp. 33-34 ◽  
Author(s):  
G. S. Shostak ◽  
H. van Woerden
Keyword(s):  
Irregular Galaxy ◽  
Ic 10

scholarly journals EVIDENCE FOR AN INTERACTION IN THE NEAREST STARBURSTING DWARF IRREGULAR GALAXY IC 10

2013 ◽  
Vol 779 (2) ◽  
pp. L15 ◽  
Author(s):  
David L. Nidever ◽  
Trisha Ashley ◽  
Colin T. Slater ◽  
Jürgen Ott ◽  
Megan Johnson ◽  
...  
Keyword(s):  
Irregular Galaxy ◽  
Ic 10

scholarly journals Stellar population of the irregular galaxy IC 10

2009 ◽  
Vol 35 (11) ◽  
pp. 748-763 ◽  
Author(s):  
N. A. Tikhonov ◽  
O. A. Galazutdinova
Keyword(s):  
Stellar Population ◽  
Irregular Galaxy ◽  
Ic 10

scholarly journals Planetary nebulae as tracers of the kinematic structure of the starburst galaxy IC 10

2011 ◽  
Vol 7 (S283) ◽  
pp. 368-369
Author(s):  
Denise R. Gonçalves ◽  
Ana M. Teodorescu ◽  
Alan Alves-Brito ◽  
Roberto H. Méndez ◽  
Laura Magrini
Keyword(s):  
Star Formation ◽  
Kinematic Analysis ◽  
Local Group ◽  
Stellar Populations ◽  
Starburst Galaxy ◽  
Kinematic Structure ◽  
Irregular Galaxy ◽  
Tidal Interactions ◽  
Ic 10 ◽  
The Galaxy

AbstractThe Local Group dwarf irregular galaxy IC 10 is the nearest starburst galaxy (at 725 kpc) and presents extended and complex HI kinematics. It is believed that IC 10 is still experiencing an intense and very recent burst of star formation, likely triggered by infalling gas from an extended envelope which is counter-rotating with respect to the galaxy proper rotation. In this contribution we summarize our preliminary results (Gonçalves et al. 2011, in prep.) obtained by performing a kinematic analysis of the PN population of IC 10. Our aim is to explore the kinematic connection of its intermediate to old stellar populations with that obtained from HI observations. Some PNe were found at large galactocentric distances and could therefore represent a trace of past tidal interactions.

Cepheid and Tip of the Red Giant Branch Distances to the Dwarf Irregular Galaxy IC 10

1999 ◽  
Vol 511 (2) ◽  
pp. 671-679 ◽  
Author(s):  
Shoko Sakai ◽  
Barry F. Madore ◽  
Wendy L. Freedman
Keyword(s):  
Irregular Galaxy ◽  
Ic 10 ◽  
Red Giant

scholarly journals HI Observations of the Irregular Galaxy IC 10

1983 ◽  
Vol 100 ◽  
pp. 33-34
Author(s):  
G. S. Shostak ◽  
H. van Woerden
Keyword(s):  
Radial Velocity ◽  
Local Group ◽  
Galactic Latitude ◽  
Irregular Galaxy ◽  
Ic 10 ◽  
Group Member

IC 10 is seen optically as a patchy nebulosity, approximately 3 × 4 arcmin in size, possibly heavily obscured due to its low (−3°) Galactic latitude. De Vaucouleurs and Freeman (1972) have classified it as a Magellanic barred irregular. With a heliocentric radial velocity of −350 km/sec, its distance is uncertain, and various investigators have placed it as far away as 3, and as near as 1 Mpc (Bottinelli et al., 1972; Roberts, 1962). For the latter value, IC 10 would be a Local Group member.

A nonthermal superbubble in the irregular galaxy IC 10

1993 ◽  
Vol 106 ◽  
pp. 1448 ◽  
Author(s):  
Hui Yang ◽  
Evan D. Skillman
Keyword(s):  
Irregular Galaxy ◽  
Ic 10

scholarly journals A Nonthermal Superbubble in the Irregular Galaxy IC 10

1988 ◽  
Vol 101 ◽  
pp. 465-467
Author(s):  
Evan D. Skillman
Keyword(s):  
High Resolution ◽  
Spectral Index ◽  
Supernova Remnant ◽  
Radio Continuum ◽  
Irregular Galaxy ◽  
Large Size ◽  
Ic 10

AbstractNew high resolution radio continuum images of the nearby irregular galaxy IC 10 have revealed a large (> 250 pc) nonthermal source. The source is roughly circular with a spectral index of ∼ –0.5, and is most likely a very large supernova remnant. Its large size suggests that it is the result of several supernovae, and may be related to the supershells observed in our own and other galaxies.

scholarly journals A kinematical search for Wolf-Rayet nebulae in the irregular galaxy IC 10

1999 ◽  
Vol 193 ◽  
pp. 474-475
Author(s):  
Almudena Bullejos ◽  
Margarita Rosado ◽  
Leonid N. Georgiev ◽  
César Esteban ◽  
J.H. Borissova
Keyword(s):  
Radial Velocity ◽  
Velocity Profiles ◽  
Irregular Galaxy ◽  
Velocity Difference ◽  
Ic 10 ◽  
Fabry Perot

In this work we report the search for nebulosities associated with the candidate Wolf-Rayet stars listed in Massey el al (1992) in the irregular galaxy IC 10, based upon Hα, [S II], and [O III] direct images and imaging Fabry-Pérot spectroscopy. Approximately 95% of the WR candidate stars we analyzed are found within nebulae. For most of these nebulae, we find broad wings on their Hα radial-velocity profiles. For some of the nebulae, the Hα velocity profiles are broadened with a typical velocity difference of 80–100 kms1.

scholarly journals A High-Resolution Radio Continuum Study Of The Dwarf Irregular Galaxy IC 10

2017 ◽  
pp. stx188 ◽  
Author(s):  
J. Westcott ◽  
E. Brinks ◽  
R.J. Beswick ◽  
V. Heesen ◽  
M.K. Argo ◽  
...  
Keyword(s):  
High Resolution ◽  
Radio Continuum ◽  
Irregular Galaxy ◽  
Ic 10

scholarly journals DEEP RADIO CONTINUUM IMAGING OF THE DWARF IRREGULAR GALAXY IC 10: TRACING STAR FORMATION AND MAGNETIC FIELDS

2011 ◽  
Vol 739 (1) ◽  
pp. L23 ◽  
Author(s):  
V. Heesen ◽  
U. Rau ◽  
M. P. Rupen ◽  
E. Brinks ◽  
D. A. Hunter
Keyword(s):  
Star Formation ◽  
Magnetic Fields ◽  
Radio Continuum ◽  
Irregular Galaxy ◽  
Ic 10
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