2016年3月16日 (三) 13:22 Shen

2016-03-16T13:22:24Z

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	'''Key Insights on Nearby Galaxies: a Far-Infrared Survey with Herschel'''		'''Key Insights on Nearby Galaxies: a Far-Infrared Survey with [[Herschel]]'''
	*The KINGFISH project is an imaging and spectroscopic survey of 61 nearby (d < 30 Mpc) galaxies, chosen to cover a wide range of galaxy properties and local interstellar medium (ISM) environments found in the Nearby Universe. Its broad goals are to characterize the ISM of present-day galaxies, the heating and cooling of their gaseous and dust components, and to better understand the physical processes linking star formation and the ISM. KINGFISH is a direct descendant of the [[Spitzer]] Infrared Nearby Galaxies Survey ([[SINGS]]), which produced complete Spitzer imaging and spectroscopic mapping and a comprehensive set of multiwavelength ancillary observations for the sample.		*The KINGFISH project is an imaging and spectroscopic survey of 61 nearby (d < 30 Mpc) galaxies, chosen to cover a wide range of galaxy properties and local interstellar medium (ISM) environments found in the Nearby Universe. Its broad goals are to characterize the ISM of present-day galaxies, the heating and cooling of their gaseous and dust components, and to better understand the physical processes linking star formation and the ISM. KINGFISH is a direct descendant of the [[Spitzer]] Infrared Nearby Galaxies Survey ([[SINGS]]), which produced complete Spitzer imaging and spectroscopic mapping and a comprehensive set of multiwavelength ancillary observations for the sample.

	*The Herschel imaging consists of complete maps for the galaxies at 70, 100, 160, 250, 350, and 500 μm. The spectral line imaging of the principal atomic ISM cooling lines ([OI]63 μm, [OIII]88 μm, [NII]122,205 μm, and [CII]158 μm) covers subregions in the centers and disks that already have been mapped in the mid-infrared with Spitzer. The KINGFISH and SINGS multi-wavelength datasets combined provide panchromatic mapping of the galaxies sufficient to resolve individual star-forming regions, and tracing the important heating and cooling channels of the ISM, across a wide range of local extragalactic ISM environments.		*The Herschel imaging consists of complete maps for the galaxies at 70, 100, 160, 250, 350, and 500 μm. The spectral line imaging of the principal atomic ISM cooling lines ([OI]63 μm, [OIII]88 μm, [NII]122,205 μm, and [CII]158 μm) covers subregions in the centers and disks that already have been mapped in the mid-infrared with Spitzer. The KINGFISH and [[SINGS]] multi-wavelength datasets combined provide panchromatic mapping of the galaxies sufficient to resolve individual star-forming regions, and tracing the important heating and cooling channels of the ISM, across a wide range of local extragalactic ISM environments.

Shen：创建页面，内容为“'''Key Insights on Nearby Galaxies: a Far-Infrared Survey with Herschel''' *The KINGFISH project is an imaging and spectroscopic survey of 61 nearby (d < 30 Mpc) gal...”

2016-03-16T13:21:49Z

创建页面，内容为“'''Key Insights on Nearby Galaxies: a Far-Infrared Survey with Herschel''' *The KINGFISH project is an imaging and spectroscopic survey of 61 nearby (d < 30 Mpc) gal...”

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'''Key Insights on Nearby Galaxies: a Far-Infrared Survey with Herschel'''
*The KINGFISH project is an imaging and spectroscopic survey of 61 nearby (d < 30 Mpc) galaxies, chosen to cover a wide range of galaxy properties and local interstellar medium (ISM) environments found in the Nearby Universe. Its broad goals are to characterize the ISM of present-day galaxies, the heating and cooling of their gaseous and dust components, and to better understand the physical processes linking star formation and the ISM. KINGFISH is a direct descendant of the [[Spitzer]] Infrared Nearby Galaxies Survey ([[SINGS]]), which produced complete Spitzer imaging and spectroscopic mapping and a comprehensive set of multiwavelength ancillary observations for the sample.

*The Herschel imaging consists of complete maps for the galaxies at 70, 100, 160, 250, 350, and 500 μm. The spectral line imaging of the principal atomic ISM cooling lines ([OI]63 μm, [OIII]88 μm, [NII]122,205 μm, and [CII]158 μm) covers subregions in the centers and disks that already have been mapped in the mid-infrared with Spitzer. The KINGFISH and SINGS multi-wavelength datasets combined provide panchromatic mapping of the galaxies sufficient to resolve individual star-forming regions, and tracing the important heating and cooling channels of the ISM, across a wide range of local extragalactic ISM environments.

KINGFISH - 版本历史

2016年3月16日 (三) 13:22 Shen

Shen：​创建页面，内容为“'''Key Insights on Nearby Galaxies: a Far-Infrared Survey with Herschel''' *The KINGFISH project is an imaging and spectroscopic survey of 61 nearby (d < 30 Mpc) gal...”

Shen：创建页面，内容为“'''Key Insights on Nearby Galaxies: a Far-Infrared Survey with Herschel''' *The KINGFISH project is an imaging and spectroscopic survey of 61 nearby (d < 30 Mpc) gal...”