Submillimeter continuum observations of Rho Ophiuchi A - The candidate protostar VLA 1623 and prestellar clumps
Protostar
Young stellar object
Submillimeter Array
Orion Nebula
DOI:
10.1086/172425
Publication Date:
2002-07-26T18:34:22Z
AUTHORS (3)
ABSTRACT
view Abstract Citations (1129) References (94) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Submillimeter Continuum Observations of rho Ophiuchi A: The Candidate Protostar VLA 1623 and Prestellar Clumps Andre, Philippe ; Ward-Thompson, Derek Barsony, Mary continuum mapping the Rho A cloud core reveals four compact clumps with masses less than about 1 solar mass embedded in an arcshaped ridge total 15 solar, lying at edge H II region around B3 star S1. Three appear amorphous shape are probably prestellar nature. fourth clump is best defined coldest coincides young stellar object (YSO) 1623. It suggested that this a protostar whose circumstellar material distributed 'cored-apple' envelope. density gradient appears to be centrally heated envelope or isothermal no central heating object. ejection extremely efficient implies global MHD approach infall outflow may required explain youngest sources. few other low-luminosity YSOs make up entirely new class YSOs. Publication: Astrophysical Journal Pub Date: March 1993 DOI: 10.1086/172425 Bibcode: 1993ApJ...406..122A Keywords: Early Stars; Protostars; Star Formation; Stellar Structure; Cosmic Dust; Energy Distribution; Waves; Astrophysics; ISM: JETS AND OUTFLOWS; INDIVIDUAL ALPHANUMERIC: 1623; STARS: CONSTELLATION NAME: RHO OPHIUCHI A; PRE--MAIN-SEQUENCE; RADIO CONTINUUM: STARS full text sources ADS | data products SIMBAD (25)
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