Some Characteristics of Current Star Formation in the 30 Doradus Nebula Revealed by [ITAL]HST[/ITAL]/NICMOS

1999 ◽  
Vol 117 (1) ◽  
pp. 225-237 ◽  
Author(s):  
Nolan R. Walborn ◽  
Rodolfo H. Barbá ◽  
Wolfgang Brandner ◽  
Mónica Rubio ◽  
Eva K. Grebel ◽  
...  
Keyword(s):  
Star Formation ◽  
30 Doradus

Infrared Studies of the Young Stellar Population of 30 Doradus

1980 ◽  
Vol 4 (1) ◽  
pp. 90-92
Author(s):  
P. J. McGregor ◽  
A. R. Hyland
Keyword(s):  
Star Formation ◽  
Stellar Population ◽  
Cluster Formation ◽  
Large Magellanic Cloud ◽  
Magellanic Cloud ◽  
Formation Processes ◽  
Excellent Opportunity ◽  
Infrared Studies ◽  
30 Doradus

The 30 Doradus region offers an excellent opportunity to study cluster formation processes and recent star formation in the Large Magellanic Cloud.

scholarly journals HST/NICMOS Survey in the 30 Doradus Nebular Filaments

1999 ◽  
Vol 190 ◽  
pp. 245-246
Author(s):  
Rodolfo H. Barbá ◽  
Nolan R. Walborn ◽  
Wolfgang Brandner ◽  
Ronald G. Probst ◽  
Mónica Rubio ◽  
...  
Keyword(s):  
Star Formation ◽  
Ample Evidence ◽  
Central Cluster ◽  
30 Doradus

On the basis of ample evidence accumulated during recent years for current star formation within the 30 Doradus Nebula, which appears to have been triggered by the massive central cluster (R136) in and just beyond the curved nebular filaments surrounding it, an HST/NICMOS survey of these regions was undertaken.

scholarly journals A New Investigation of the 30 Doradus Region with the Australia Telescope Compact Array

1999 ◽  
Vol 190 ◽  
pp. 251-253
Author(s):  
J. S. Lazendic ◽  
R. F. Haynes ◽  
J. R. Dickel ◽  
P. A. Jones ◽  
G. L. White ◽  
...  
Keyword(s):  
Star Formation ◽  
Supernova Remnants ◽  
Massive Stars ◽  
Large Magellanic Cloud ◽  
Complex Nature ◽  
Active Star ◽  
H Ii Region ◽  
The Impact ◽  
Compact Array ◽  
30 Doradus

30 Doradus is a giant H II region in the Large Magellanic Cloud (Bode 1801). It is the nearest extragalactic giant H II region and the location of active star formation. The complex nature of this extended region provides an excellent opportunity to investigate the impact of massive stars on the structure of the interstellar medium. Specifically the presence of supernova remnants (SNRs) is expected to play an important role.

scholarly journals HUBBLE TARANTULA TREASURY PROJECT. III. PHOTOMETRIC CATALOG AND RESULTING CONSTRAINTS ON THE PROGRESSION OF STAR FORMATION IN THE 30 DORADUS REGION

2016 ◽  
Vol 222 (1) ◽  
pp. 11 ◽  
Author(s):  
E. Sabbi ◽  
D. J. Lennon ◽  
J. Anderson ◽  
M. Cignoni ◽  
R. P. van der Marel ◽  
...  
Keyword(s):  
Star Formation ◽  
30 Doradus

scholarly journals HUBBLE TARANTULA TREASURY PROJECT. II. THE STAR-FORMATION HISTORY OF THE STARBURST REGION NGC 2070 IN 30 DORADUS

2015 ◽  
Vol 811 (2) ◽  
pp. 76 ◽  
Author(s):  
M. Cignoni ◽  
E. Sabbi ◽  
R. P. van der Marel ◽  
M. Tosi ◽  
D. Zaritsky ◽  
...  
Keyword(s):  
Star Formation ◽  
Star Formation History ◽  
Formation History ◽  
History Of ◽  
30 Doradus

Recent massive star formation in 30 Doradus

1987 ◽  
Vol 323 ◽  
pp. L65 ◽  
Author(s):  
Nolan R. Walborn ◽  
J. Chris Blades
Keyword(s):  
Star Formation ◽  
Massive Star ◽  
Massive Star Formation ◽  
30 Doradus

Violent Star Formation in 30 Doradus

1994 ◽  
pp. 1-12 ◽  
Author(s):  
R. C. Kennicutt ◽  
Y.-H. Chu
Keyword(s):  
Star Formation ◽  
30 Doradus

scholarly journals Dissecting 30 Doradus: Optical and Near Infrared Star Formation History of the starburst cluster NGC2070 from the Hubble Tarantula Treasury Project

2015 ◽  
Vol 12 (S316) ◽  
pp. 77-83
Author(s):  
Michele Cignoni ◽  
Keyword(s):  
Star Formation ◽  
Main Sequence ◽  
Near Infrared ◽  
Mass Function ◽  
Large Magellanic Cloud ◽  
Initial Mass Function ◽  
Star Formation History ◽  
Formation History ◽  
History Of ◽  
30 Doradus

AbstractI will present new results on the star formation history of 30 Doradus in the Large Magellanic Cloud based on the panchromatic imaging survey Hubble Tarantula Treasury Project (HTTP). Here the focus is on the starburst cluster NGC2070. The star formation history is derived by comparing the deepest ever optical and NIR color-magnitude diagrams (CMDs) with state-of-the-art synthetic CMDs generated with the latest PARSEC models, which include all stellar phases from pre-main sequence to post-main sequence. For the first time in this region we are able to measure the star formation using intermediate and low mass stars simultaneously. Our results suggest that NGC2070 experienced a prolonged activity. I will discuss the detailed star formation history, initial mass function and reddening distribution.

scholarly journals A STUDY OF THE RELATION BETWEEN STAR FORMATION AND MOLECULAR CLUMPS ON SUBPARSEC SCALES IN 30 DORADUS

2016 ◽  
Vol 831 (1) ◽  
pp. 32 ◽  
Author(s):  
O. Nayak ◽  
M. Meixner ◽  
R. Indebetouw ◽  
G. De Marchi ◽  
A. Koekemoer ◽  
...  
Keyword(s):  
Star Formation ◽  
30 Doradus

Infrared Observations of Ongoing Star Formation in the 30 Doradus Nebula and a Comparison with [ITAL]Hubble[/ITAL] [ITAL]Space[/ITAL] [ITAL]T[/ITAL][ITAL]elescope[/ITAL] WFPC2 Images

1998 ◽  
Vol 116 (4) ◽  
pp. 1708-1718 ◽  
Author(s):  
Mónica Rubio ◽  
Rodolfo H. Barbá ◽  
Nolan R. Walborn ◽  
Ronald G. Probst ◽  
Jorge García ◽  
...  
Keyword(s):  
Star Formation ◽  
Infrared Observations ◽  
30 Doradus
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