scholarly journals H II REGIONS: WITNESSES TO MASSIVE STAR FORMATION

2010 ◽  
Vol 711 (2) ◽  
pp. 1017-1028 ◽  
Author(s):  
Thomas Peters ◽  
Robi Banerjee ◽  
Ralf S. Klessen ◽  
Mordecai-Mark Mac Low ◽  
Roberto Galván-Madrid ◽  
...  
2008 ◽  
Vol 482 (2) ◽  
pp. 585-596 ◽  
Author(s):  
L. Deharveng ◽  
B. Lefloch ◽  
S. Kurtz ◽  
D. Nadeau ◽  
M. Pomarès ◽  
...  

Galaxies ◽  
2020 ◽  
Vol 8 (1) ◽  
pp. 13 ◽  
Author(s):  
Claus Leitherer

Spectroscopic observations of a massive star formation in the ultraviolet and their interpretation are reviewed. After a brief historical retrospective, two well-studied resolved star clusters and the surrounding H II regions are introduced: NGC 2070 in the Large Magellanic Cloud and NGC 604 in M33. These regions serve as a training set for studies of more distant clusters, which can no longer be resolved into individual stars. Observations of recently formed star clusters and extended regions in star-forming galaxies in the nearby universe beyond the Local Group are presented. Their interpretation relies on spectral synthesis models. The successes and failures of such models are discussed, and future directions are highlighted. I present a case study of the extraordinary star cluster and giant H II region in the blue compact galaxy II Zw 40. The review concludes with a preview of two upcoming Hubble Space Telescope programs: ULLYSES, a survey of massive stars in nearby galaxies, and CLASSY, a study of massive star clusters in star-forming galaxies.


2006 ◽  
Vol 446 (1) ◽  
pp. 171-184 ◽  
Author(s):  
A. Zavagno ◽  
L. Deharveng ◽  
F. Comerón ◽  
J. Brand ◽  
F. Massi ◽  
...  

2010 ◽  
Vol 725 (2) ◽  
pp. 1429-1439 ◽  
Author(s):  
F. Yusef-Zadeh ◽  
J. H. Lacy ◽  
M. Wardle ◽  
B. Whitney ◽  
H. Bushouse ◽  
...  

2005 ◽  
Vol 433 (2) ◽  
pp. 565-577 ◽  
Author(s):  
L. Deharveng ◽  
A. Zavagno ◽  
J. Caplan

2006 ◽  
Vol 458 (1) ◽  
pp. 191-201 ◽  
Author(s):  
L. Deharveng ◽  
B. Lefloch ◽  
F. Massi ◽  
J. Brand ◽  
S. Kurtz ◽  
...  

2019 ◽  
Vol 489 (4) ◽  
pp. 5530-5546 ◽  
Author(s):  
L Rousseau-Nepton ◽  
R P Martin ◽  
C Robert ◽  
L Drissen ◽  
P Amram ◽  
...  

ABSTRACT SIGNALS, the Star formation, Ionized Gas, and Nebular Abundances Legacy Survey, is a large observing programme designed to investigate massive star formation and H ii regions in a sample of local extended galaxies. The programme will use the imaging Fourier transform spectrograph SITELLE at the Canada–France–Hawaii Telescope. Over 355 h (54.7 nights) have been allocated beginning in fall 2018 for eight consecutive semesters. Once completed, SIGNALS will provide a statistically reliable laboratory to investigate massive star formation, including over 50 000 resolved H ii regions: the largest, most complete, and homogeneous data base of spectroscopically and spatially resolved extragalactic H ii regions ever assembled. For each field observed, three datacubes covering the spectral bands of the filters SN1 (363–386 nm), SN2 (482–513 nm), and SN3 (647–685 nm) are gathered. The spectral resolution selected for each spectral band is 1000, 1000, and 5000, respectively. As defined, the project sample will facilitate the study of small-scale nebular physics and many other phenomena linked to star formation at a mean spatial resolution of ∼20 pc. This survey also has considerable legacy value for additional topics, including planetary nebulae, diffuse ionized gas, and supernova remnants. The purpose of this paper is to present a general outlook of the survey, notably the observing strategy, galaxy sample, and science requirements.


2015 ◽  
Vol 451 (2) ◽  
pp. 1307-1330 ◽  
Author(s):  
Javier Zaragoza-Cardiel ◽  
John E. Beckman ◽  
Joan Font ◽  
Begoña García-Lorenzo ◽  
Artemi Camps-Fariña ◽  
...  

2016 ◽  
Vol 818 (1) ◽  
pp. 52 ◽  
Author(s):  
Kei E. I. Tanaka ◽  
Jonathan C. Tan ◽  
Yichen Zhang

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