Results 71 to 80 of about 1,290 (180)
Dome C observations of massive protostars
The importance of a Dome C facility for studies of massive star formation is highlighted. Using an example of a statistical study of 380 candidate massive protostars based on the GLIMPSE legacy program data from the Spitzer Space Telescope, the ...
M.S.N. Kumar
core +1 more source
SpectacularSpitzerImages of the Trifid Nebula: Protostars in a Young, Massive‐Star‐forming Region
Spitzer IRAC and MIPS images of the Trifid Nebula (M20) reveal its spectacular appearance in infrared light, highlighting the nebula's special evolutionary stage. The images feature recently-formed massive protostars and numerous young stellar objects, and a single O star that illuminates the surrounding molecular cloud from which it formed, and unveil
Rho, Jeonghee +3 more
openaire +3 more sources
SGG acknowledges support from the Science & Technology Facilities Council (STFC) via an Ernest Rutherford Fellowship [ST/J003255/1]. SHPA acknowledges financial support from CNPq, CAPES and Fapemig.We report results of a spectropolarimetric and ...
Delfosse, X. +47 more
core +1 more source
Dissecting high-mass protostars with SPARKS
The origin of the highest mass stars is still an enigma in modern astrophysics. The SPARKS project (Search for high-mass protostars with ALMA up to 5 kpc) is a high angular resolution follow-up of the complete sample of infrared quiet massive clumps ...
Csengeri, Timea +1 more
core +1 more source
Search for Binary Protostars [PDF]
In an effort to shed more light on the formation process of binary stars, we have started a program to study multiplicity among nearby low- and intermediate-mass protostars using the OVRO Millimeter Array.
Launhardt, R. +2 more
core
In this lecture, we briefly present the main models currently proposed to describe the collapse of prestellar dense cores and the formation of young Class 0 protostars.
A. Maury
core +1 more source
Proceedings of Protostars and Planets V
Oral presentation sessions in this conference include: Clouds and cores; Star formation and protostars; Binaries and multiples; Newborn massive stars; jets and outflows; Clusters and associations; T Tauri stars and disks; Brown dwarfs; Planet formation ...
core
Disentangling the Formation Pathways of Protostars [PDF]
Star formation occurs within dense cores within molecular clouds, often associated with filamentary structures. However, there exist isolated instances of star formation, far from nearby forming stars.
Reynolds Tran, Nickalas
core
Variability of Deeply Embedded Protostars: A New Direction for Star Formation?
The formation of a star is a dynamic process fed by the gravitational collapse of a molecular cloud core. Theoretical models and observations suggest that the majority of this infalling material settles into a protoplanetary disk before reaching the (proto)star and therefore that disk accretion processes are responsible for the rate at which the (proto)
openaire +2 more sources
From Pre-Stellar Cores to Protostars: The Initial Conditions of Star Formation
TeX file, 37 pages, 8 figures, 1 Table - To appear in Protostars & Planets IV, eds. V. Mannings, A. Boss, S. Russell (Tucson: The University of Arizona Press)
Andre, Philippe +2 more
openaire +2 more sources

