scholarly journals Massive Star Formation and Evolution in Starburst Galaxies: Mid‐infrared Spectroscopy with theISOShort Wavelength Spectrometer

2000 ◽  
Vol 539 (2) ◽  
pp. 641-657 ◽  
Author(s):  
Michele D. Thornley ◽  
Natascha M. Forster Schreiber ◽  
Dieter Lutz ◽  
Reinhard Genzel ◽  
Henrik W. W. Spoon ◽  
...  
1986 ◽  
Vol 116 ◽  
pp. 523-528
Author(s):  
J. A. Graham ◽  
Taft E. Armandroff

Highlights of the IAU Symposium 116 are reviewed. Some of the general themes running through the meeting are identified. These include:i) the fruitful interaction between observation, laboratory work and theory. ii) the need for understanding and, if possible, correcting for the effects of incompleteness and bias in observing lists. iii) the importance of the Magellanic Clouds, as the nearest independently evolving stellar systems, in the study of massive star formation and evolution in galaxies.


2003 ◽  
Vol 287 (1-4) ◽  
pp. 191-194 ◽  
Author(s):  
M.S. Nanda Kumar ◽  
Christopher J. Davis ◽  
Rafael Bachiller

2009 ◽  
Vol 699 (1) ◽  
pp. 667-685 ◽  
Author(s):  
Karín Menéndez-Delmestre ◽  
Andrew W. Blain ◽  
Ian Smail ◽  
Dave M. Alexander ◽  
Scott C. Chapman ◽  
...  

2000 ◽  
Vol 119 (1) ◽  
pp. 79-93 ◽  
Author(s):  
Christopher J. Conselice ◽  
John S. Gallagher ◽  
Daniela Calzetti ◽  
Nicole Homeier ◽  
Anne Kinney

2008 ◽  
Vol 4 (S256) ◽  
pp. 343-348
Author(s):  
Alceste Z. Bonanos

AbstractDespite the large impact very massive stars (>30 M⊙) have in astrophysics, their fundamental parameters remain uncertain. I present results of a survey aiming to characterize the most massive stars in the Magellanic Clouds. The survey targets the brightest, blue, eclipsing binaries discovered by the OGLE microlensing survey, for which masses and radii are measured to 5%. Such precise data are rare and provide constraints for theories of massive star formation and evolution at low metallicities.


1992 ◽  
Vol 45 (4) ◽  
pp. 389
Author(s):  
Colin A Norman

The observations relevant to star formation at high redshift are reviewed including radio galaxies, quasars, IRAS objects, and QSO emission and absorption line regions. Low redshift counterparts associated with starburst galaxies are discussed. The relation of galaxy formation, starbursts, and active galaxies and quasars is briefly reviewed. The role of feedback in galaxy formation and massive star formation is briefly analysed.


1999 ◽  
Vol 193 ◽  
pp. 739-740
Author(s):  
Duíla F. de Mello ◽  
Marcio A.G. Maia ◽  
Daniel Schaerer ◽  
Claus Leitherer

In order to study the influence of the environment in galaxies we have selected a sample from the catalog by Maia et al. (1994) which contains objects in low and high density areas of the Southern sky. These samples have been observed with the Brazilian-ESO 1.52m telescope and long-slit spectra are being analyzed. With our database we will be able to investigate the role of the environment in the galaxy population. We will be able to search for WR features and massive stars. It is our goal to compare the general properties of these galaxies with typical starburst galaxies which are dominated by episodes of massive star formation.


2007 ◽  
Vol 669 (1) ◽  
pp. 464-482 ◽  
Author(s):  
D. S. Shepherd ◽  
M. S. Povich ◽  
B. A. Whitney ◽  
T. P. Robitaille ◽  
D. E. A. Nurnberger ◽  
...  

2013 ◽  
Vol 9 (S303) ◽  
pp. 220-222
Author(s):  
Sarah Kendrew ◽  
Adam Ginsburg ◽  
Katharine Johnston ◽  
Henrik Beuther ◽  
John Bally ◽  
...  

AbstractWe summarize here our recent findings from near-infrared spectroscopy and 1 mm line and continuum observations of a recently identified extended green object (EGO) in Sgr C, whose observational characteristics suggest early-stage massive star formation is taking place. Located on the outskirts of the massive evolved Hii region associated with Sgr C in the Western central molecular zone (CMZ), the EGO measures ∼10″ (0.4 pc at 8.5 kpc). We confirm that early-stage star formation is taking place on the periphery of the Sgr C Hii region. The data show clear detections of two protostellar cores and several knots of H2 and Brackett γ emission alongside a previously detected compact radio source. We calculate the cores' joint mass to be ∼103 M⊙, with column densities of 1-2 × 1024 cm−2. The host molecular clouds mass is approximately 105 M⊙. Despite these favorable conditions, the cloud is curiously devoid of any further star formation, making it comparable to other remarkably quiescent clouds, such as G0.253 in the Eastern CMZ.


Sign in / Sign up

Export Citation Format

Share Document