Proto-Planetary Disk and Planetary Formation Takayuki Tanigawa.
Spin-Orbit Misalignment in Planetary Systems and Magnetic Star -- Disk Interaction IAU Astrophysics of Planetary Systems, Torino, Italy, Oct.14, 2010 Dong.
Tsuribe, T. (Osaka U.) Cloud Fragmentation via filament formation Introduction Basic Aspects of Cloud Fragmentation Application to the Metal deficient.
Variability of Be Stars: A Key to the Structure of their Circumstellar Environments Anatoly Miroshnichenko University of Toledo Variable Star Meeting 2004.
How do massive stars form? A comparison of model tracks with Herschel data Michael D Smith CAPS University of Kent Available at: //astro.kent.ac.uk/mds/capsule.pdf.
I N T R O D U C T I O N The mechanism of galaxy formation involves the cooling and condensation of baryons inside the gravitational potential well provided.
Anti-Correlated Lags in Compact Stellar X-ray Sources Dr. Kandulapati Sriram Collaborators: Prof A. R. Rao (TIFR) Dr. Vivek Kumar Agrawal (ISRO/TIFR).
Summary Talk
Tsuribe, T. (Osaka U.)
Summary Talk Andrea Ferrara 4C - Center for Computational Chemistry and Cosmology Scuola Normale Superiore, Pisa, Italy & Kavli IPMU, Tokyo, Japan.
Gravitational Collapse and Disk Formation in Magnetized Cores Susana Lizano CRyA, UNAM Transformational Science with ALMA: From Dust to Rocks to Planets,
Phys 778 – 2009 2. Molecular Clouds
