The process that leads to the formation of the bright star-forming sites observed along prominent spiral arms remains elusive. We present results of a multi-wavelength study of a spiral arm segment in the nearby grand-design spiral galaxy M51 that belongs to a spiral density wave and exhibits nine gas spurs. The combined observations of the (ionized, atomic, molecular, dusty) interstellar medium with star formation tracers (H II regions, young <10 Myr stellar clusters) suggest (1) no variation in giant molecular cloud (GMC) properties between arm and gas spurs, (2) gas spurs and extinction feathers arising from the same structure with a close spatial relation between gas spurs and ongoing/recent star formation (despite higher gas surface de...
Spiral arm spurs are prominent features that have been observed in extinction and 8 m emission in ne...
The origin and types of spiral arms are reviewed with an emphasis on the connections between these a...
Spiral arm spurs are prominent features that have been observed in extinction and 8 m emission in ne...
The process that leads to the formation of the bright star-forming sites observed along prominent sp...
What role does Galactic structure play in star formation? We have used the Herschel Infrared Galacti...
What role does Galactic structure play in star formation? We have used the Herschel Infrared Galacti...
This is the final version of the article. Available fromAmerican Astronomical Society / IOP Publishi...
Using data from the PdBI Arcsecond Whirlpool Survey (PAWS), we have generated the largest extragalac...
Using data from the PdBI Arcsecond Whirlpool Survey (PAWS), we have generated the largest extragalac...
What role does Galactic structure play in star formation? We have used the Herschel Infrared Galacti...
What role does Galactic structure play in star formation? We have used the Herschel Infrared Galacti...
Abstract. Studying star formation in spiral arms tells us not only about the evolution of star forma...
What role does Galactic structure play in star formation? We have used the Herschel Hi-GAL compact-c...
The Plateau de Bure Interferometer Arcsecond Whirlpool Survey has mapped the molecular gas in the ce...
We study star formation processes in the disc of the weakly barred grand design spiral galaxy M100 (...
Spiral arm spurs are prominent features that have been observed in extinction and 8 m emission in ne...
The origin and types of spiral arms are reviewed with an emphasis on the connections between these a...
Spiral arm spurs are prominent features that have been observed in extinction and 8 m emission in ne...
The process that leads to the formation of the bright star-forming sites observed along prominent sp...
What role does Galactic structure play in star formation? We have used the Herschel Infrared Galacti...
What role does Galactic structure play in star formation? We have used the Herschel Infrared Galacti...
This is the final version of the article. Available fromAmerican Astronomical Society / IOP Publishi...
Using data from the PdBI Arcsecond Whirlpool Survey (PAWS), we have generated the largest extragalac...
Using data from the PdBI Arcsecond Whirlpool Survey (PAWS), we have generated the largest extragalac...
What role does Galactic structure play in star formation? We have used the Herschel Infrared Galacti...
What role does Galactic structure play in star formation? We have used the Herschel Infrared Galacti...
Abstract. Studying star formation in spiral arms tells us not only about the evolution of star forma...
What role does Galactic structure play in star formation? We have used the Herschel Hi-GAL compact-c...
The Plateau de Bure Interferometer Arcsecond Whirlpool Survey has mapped the molecular gas in the ce...
We study star formation processes in the disc of the weakly barred grand design spiral galaxy M100 (...
Spiral arm spurs are prominent features that have been observed in extinction and 8 m emission in ne...
The origin and types of spiral arms are reviewed with an emphasis on the connections between these a...
Spiral arm spurs are prominent features that have been observed in extinction and 8 m emission in ne...