Propagation of highly_efficient_star_formation_in_ngc7000
Lyα Pumped Molecular Hydrogen Emission in the Planetary Nebulae NGC 6853 and NGC 3132 R.E. Lupu, K. France and S.R. McCandliss Johns Hopkins University,
YSOs: Young Stellar Objects Provide evidence for planet-forming nebular disks around stars Dusty cocoon surrounding YSO.
21 Mars 2006Visions for infrared astronomy1 Protoplanetary worlds at the AU scale Jean Philippe Berger J. Monnier, R. Millan-Gabet, W. Traub, M. Benisty,
FUSE LWRS aperture overlays on the NGC 6853 VLT 8.2-m image, obtained from ESO.
Protoplanetary disks as seen by the IRAM array Vincent Pietu (LAOG) A few important points in the observations and analysis related to the survey we have.
In a dense molecular cloud far, far away M16: The Eagle Nebula Dense Molecular gas Hot, ionized gas Young stars.
Five Systems with IRAC Excesses RX J1111.7-7620 Cham. I member, ~3 Myr old, not actively accreting? [PZ99] RXS J161411-230536 Upper-Scorpius OB association,
Study of Planet forming Systems Orbiting Intermediate-mass Stars Sweta Shah Ithaca College Advisor: Dr. Luke Keller In collaboration with the NASA Spitzer.
Study of Planet forming Systems Orbiting Intermediate-mass Stars
Most meteorites formed in the earliest moments of solar system history Early solar system consisted of a planetary nebula-- dust and gas surrounding protostar.
Sternentstehung - Star Formation
![Five Systems with IRAC Excesses RX J1111.7-7620 Cham. I member, ~3 Myr old, not actively accreting? [PZ99] RXS J161411-230536 Upper-Scorpius OB association,](https://static.fdocuments.in/doc/330x215/56649ea95503460f94bacdf7/five-systems-with-irac-excesses-rx-j11117-7620-cham-i-member-3-myr-old.jpg)
