Perspectives of Space Submillimeter Astronomy
St. Petersburg, Russia, 30 September - 2 October, 2002

Viewgaphs of the presentation

	I.I. Zinchenko Submillimeter studies of star-forming regions
	Slide02 Contents
	Slide03 Submm band is the last relatively unexplored part of electromagnetic spectrum.
	Slide04 The spectrum of Sgr B2
	Slide05 Scientific importance of millimeter and submillimeter astronomy
	Slide06 Multi-frequency HNCO survey
	Slide07 Detection of HD
	Slide08 Detection of triply deuterated ammonia
	Slide09 Basic physical properties of HMSF cores
	Slide10 Scientific tasks for submm observations of star forming regions from space
	Slide11 Search for star-forming cores
	Slide12 Line versus continuum surveys
	Slide13 A detailed map of G268.42-0.85 in HCO+(4–3)
	Slide14 Structure of star forming regions: S76E
	Slide15 Chemical differentiations in regions of high mass star formation
	Slide16 Polarization of dust emission and magnetic fields in star forming regions
	Slide17 Astrochemistry and chemical evolution in star forming regions
	Slide18 CSO submm line surveys
	Slide19 Spectra of three low-mass YSOs at different evolutionary stages.
	Slide20 Shock diagnostics
	Slide21 Some important submillimeter atomic and molecular transitions
	Slide22 Transparency of the atmosphere in the submillimeter wave range
	Slide23 Dependence on precipitable water vapor
	Slide24 Submillimeter wave receivers
	Slide25 Noise temperature for different types of receivers
	Slide26 Noise temperature of HEB receivers
	Slide27 Conclusions