scholarly journals Progress in 2012-2013 on HEDLP LAB 11-583 Eagle Nebula

2013 ◽  
Author(s):  
J Kane
Keyword(s):  
Eagle Nebula

scholarly journals Pre-main-sequence stars older than 8 Myr in the Eagle nebula

2013 ◽  
Vol 435 (4) ◽  
pp. 3058-3070 ◽  
Author(s):  
Guido De Marchi ◽  
Nino Panagia ◽  
M. G. Guarcello ◽  
Rosaria Bonito
Keyword(s):  
Main Sequence ◽  
Main Sequence Stars ◽  
Eagle Nebula

Eagle Nebula Pillars: From Models to Observations

2005 ◽  
pp. 177-181
Author(s):  
Marc W. Pound ◽  
Jave O. Kane ◽  
Bruce A. Remington ◽  
Dmitri D. Ryutov ◽  
Akira Mizuta ◽  
...  
Keyword(s):  
Eagle Nebula

scholarly journals FOREST unbiased Galactic plane imaging survey with the Nobeyama 45 m telescope (FUGIN). VIII. Possible evidence of cloud–cloud collisions triggering high-mass star formation in the giant molecular cloud M 16 (Eagle Nebula)

2020 ◽  
Author(s):  
Atsushi Nishimura ◽  
Shinji Fujita ◽  
Mikito Kohno ◽  
Daichi Tsutsumi ◽  
Tetsuhiro Minamidani ◽  
...  
Keyword(s):  
Star Formation ◽  
Molecular Cloud ◽  
Velocity Structure ◽  
Galactic Plane ◽  
High Mass ◽  
Mass Star ◽  
Collision Event ◽  
Giant Molecular Cloud ◽  
Eagle Nebula ◽  
H Ii Region

Abstract M 16, the Eagle Nebula, is an outstanding H ii region which exhibits extensive high-mass star formation and hosts remarkable “pillars.” We herein obtained new 12COJ = 1–0 data for the region observed with NANTEN2, which were combined with the 12COJ = 1–0 data obtained using the FOREST unbiased galactic plane imaging with Nobeyama 45 m telescope (FUGIN) survey. These observations revealed that a giant molecular cloud (GMC) of ∼1.3 × 105 M⊙ is associated with M 16, which extends for 30 pc perpendicularly to the galactic plane, at a distance of 1.8 kpc. This GMC can be divided into the northern (N) cloud, the eastern (E) filament, the southeastern (SE) cloud, the southeastern (SE) filament, and the southern (S) cloud. We also found two velocity components (blueshifted and redshifted components) in the N cloud. The blueshifted component shows a ring-like structure, and the redshifted one coincides with the intensity depression of the ring-like structure. The position–velocity diagram of the components showed a V-shaped velocity feature. The spatial and velocity structures of the cloud indicated that two different velocity components collided with each other at a relative velocity of 11.6 km s−1. The timescale of the collision was estimated to be ∼4 × 105 yr. The collision event reasonably explains the formation of the O9V star ALS 15348, as well as the shape of the Spitzer bubble N19. A similar velocity structure was found in the SE cloud, which is associated with the O7.5V star HD 168504. In addition, the complementary distributions of the two velocity components found in the entire GMC suggested that the collision event occurred globally. On the basis of the above results, we herein propose a hypothesis that the collision between the two components occurred sequentially over the last several 106 yr and triggered the formation of O-type stars in the NGC 6611 cluster in M 16.

scholarly journals ChandraObservations of the Eagle Nebula. I. Embedded Young Stellar Objects near the Pillars of Creation

2007 ◽  
Vol 654 (1) ◽  
pp. 347-360 ◽  
Author(s):  
Jeffrey L. Linsky ◽  
Marc Gagne ◽  
Anna Mytyk ◽  
Mark McCaughrean ◽  
Morten Andersen
Keyword(s):  
Young Stellar Objects ◽  
Stellar Objects ◽  
Eagle Nebula

scholarly journals Embedded Star Formation in the Eagle Nebula withSpitzerGLIMPSE

2007 ◽  
Vol 666 (1) ◽  
pp. 321-338 ◽  
Author(s):  
R. Indebetouw ◽  
T. P. Robitaille ◽  
B. A. Whitney ◽  
E. Churchwell ◽  
B. Babler ◽  
...  
Keyword(s):  
Star Formation ◽  
Eagle Nebula

scholarly journals Tracing the energetics and evolution of dust withSpitzer: a chapter in the history of the Eagle Nebula

2011 ◽  
Vol 531 ◽  
pp. A51 ◽  
Author(s):  
N. Flagey ◽  
F. Boulanger ◽  
A. Noriega-Crespo ◽  
R. Paladini ◽  
T. Montmerle ◽  
...  
Keyword(s):  
Eagle Nebula ◽  
History Of

scholarly journals Pre-main sequence stars with disks in the Eagle Nebula observed in scattered light

2010 ◽  
Vol 521 ◽  
pp. A18 ◽  
Author(s):  
M. G. Guarcello ◽  
F. Damiani ◽  
G. Micela ◽  
G. Peres ◽  
L. Prisinzano ◽  
...  
Keyword(s):  
Main Sequence ◽  
Scattered Light ◽  
Main Sequence Stars ◽  
Eagle Nebula

scholarly journals Near-Infrared Polarimetry of the Eagle Nebula (M 16)

2007 ◽  
Vol 59 (3) ◽  
pp. 507-517 ◽  
Author(s):  
Koji Sugitani ◽  
Makoto Watanabe ◽  
Motohide Tamura ◽  
Ryo Kandori ◽  
James H. Hough ◽  
...  
Keyword(s):  
Near Infrared ◽  
Eagle Nebula
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