ORIGIN OF THE GALACTIC CENTER S-STARS: GRAVITATIONAL TORQUES FROM LIN-SHU-TYPE SPIRAL DENSITY WAVES
- Department of Physics, Ben-Gurion University, P.O. Box 653, Beer-Sheva 84105 (Israel)
The supermassive approx4 x 10{sup 6} M{sub sun} black hole at the Galactic center is surrounded by a parsec-scale star disk, with several thousands of dynamically relaxed, evolved, late-type CO absorption line stars and a small approx100 population of luminous O and Wolf-Rayet stars which move in approximately circular Keplerian orbits. These bluish in color massive O and Wolf-Rayet stars are very young with an estimated age of 6 +- 2 Myr. Another small group of roughly 20 young (<10 Myr) blue B stars with the orbital periods as short as 15 years ('S-stars') follow eccentric, randomly oriented orbits well inside the disk stars. A model is proposed to explain the S-stars. Accordingly, the stars formed originally in the parsec-scale disk through Jeans' gravitational fragmentation of gas. The newly formed S-stars then migrated inward to the Galactic center via the torques exerted by Lin-Shu-type spiral density waves on the stars at an inner Lindblad resonance. The model explains both the number of observed S-stars orbiting the Galactic black hole within the nuclear (<0.05 pc) star cluster and the key property of the S-star orbits, namely, their high eccentricities.
- OSTI ID:
- 21392311
- Journal Information:
- Astrophysical Journal, Vol. 709, Issue 2; Other Information: DOI: 10.1088/0004-637X/709/2/597; ISSN 0004-637X
- Country of Publication:
- United States
- Language:
- English
Similar Records
A RAPIDLY EVOLVING REGION IN THE GALACTIC CENTER: WHY S-STARS THERMALIZE AND MORE MASSIVE STARS ARE MISSING
DYNAMICAL CONSTRAINTS ON THE ORIGIN OF THE YOUNG B-STARS IN THE GALACTIC CENTER
Related Subjects
COSMOLOGY AND ASTRONOMY
ABSORPTION
BLACK HOLES
CARBON MONOXIDE
COLOR
GALAXIES
ORBITS
STAR CLUSTERS
TORQUE
WOLF-RAYET STARS
CARBON COMPOUNDS
CARBON OXIDES
CHALCOGENIDES
MAIN SEQUENCE STARS
OPTICAL PROPERTIES
ORGANOLEPTIC PROPERTIES
OXIDES
OXYGEN COMPOUNDS
PHYSICAL PROPERTIES
SORPTION
STARS