Astronomy and Astrophysics – Astronomy
Scientific paper
Jul 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.217..201a&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 217, no. 1-2, p. 201-206
Astronomy and Astrophysics
Astronomy
Accretion Disks, Galaxies, Infrared Astronomy, Sky Surveys (Astronomy), Star Formation, Stellar Mass, T Tauri Stars, Angular Momentum, Energy Distribution, Fragmentation, Interstellar Magnetic Fields, Rates (Per Time), Stellar Physics, Stellar Winds
Scientific paper
Star forming regions and young stellar objects are well known to be strong sources of infrared radiation. Such objects will be among the conspicuous targets in the upcoming Near-Infrared (NIR) surveys. Therefore, these surveys promise important new information on various unsolved questions concerning the star formation process. Among the problems where significant progress can be expected are the environmental effects on star formation, the derivation of star formation efficiencies and star formation rates, and all questions related to the fragmentation process and the initial mass function. Moreover, the NIR surveys may also help identifying new examples of protostars and Pre-Main Sequence (PMS) objects for follow-up investigations of their physical structure.
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