"synopsis" may belong to another edition of this title.
The most massive stars in the galaxy - those with more than 15 to 20 solar masses - are lilkely to ionize their surroundings before they reach their final mass. How can they accrete in spite of the presence of over-pressurized gas?
This thesis presents results of Submillimeter Array (SMA) and Very Large Array (VLA) studies of massive star formation regions in the early stages of ionization, as well as an analysis of numerical simulations of the evolution of these young HII regions. The results favor a picture in which very massive stars form in accretion flows that are partially ionized and that keep accreting material from their environment.
The American Astronomical Society selected Roberto Galvan-Madrid as a prize winner for The Rodger Doxsey Travel Prize in 2010.
"About this title" may belong to another edition of this title.
Book Description Soft Cover. Condition: new. This item is printed on demand. Seller Inventory # 9781461433071
Book Description Condition: New. Seller Inventory # ABLIING23Mar2716030036153
Book Description Condition: New. Seller Inventory # 17848429-n
Book Description Condition: New. PRINT ON DEMAND Book; New; Fast Shipping from the UK. No. book. Seller Inventory # ria9781461433071_lsuk
Book Description Paperback. Condition: Brand New. 2012 edition. 135 pages. 9.25x6.25x0.25 inches. In Stock. Seller Inventory # x-146143307X
Book Description Paperback / softback. Condition: New. This item is printed on demand. New copy - Usually dispatched within 5-9 working days. Seller Inventory # C9781461433071
Book Description Condition: New. Seller Inventory # 17848429-n
Book Description Taschenbuch. Condition: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -The most massive stars in the galaxy - those with more than 15 to 20 solar masses - are lilkely to ionize their surroundings before they reach their final mass. How can they accrete in spite of the presence of over-pressurized gas This thesis presents results of Submillimeter Array (SMA) and Very Large Array (VLA) studies of massive star formation regions in the early stages of ionization, as well as an analysis of numerical simulations of the evolution of these young HII regions. The results favor a picture in which very massive stars form in accretion flows that are partially ionized and that keep accreting material from their environment. 136 pp. Englisch. Seller Inventory # 9781461433071
Book Description Condition: New. This book presents results of Submillimeter Array (SMA) and Very Large Array (VLA) studies of massive-star formation regions in the early stages of ionization. Series: Springer Theses. Num Pages: 135 pages, 26 black & white illustrations, 23 colour illustrations, 9 black & white tables, biograph. BIC Classification: PGC. Category: (P) Professional & Vocational. Dimension: 235 x 155 x 8. Weight in Grams: 219. . 2012. Paperback. . . . . Seller Inventory # V9781461433071
Book Description Taschenbuch. Condition: Neu. Druck auf Anfrage Neuware - Printed after ordering - The most massive stars in the galaxy - those with more than 15 to 20 solar masses - are lilkely to ionize their surroundings before they reach their final mass. How can they accrete in spite of the presence of over-pressurized gas This thesis presents results of Submillimeter Array (SMA) and Very Large Array (VLA) studies of massive star formation regions in the early stages of ionization, as well as an analysis of numerical simulations of the evolution of these young HII regions. The results favor a picture in which very massive stars form in accretion flows that are partially ionized and that keep accreting material from their environment. Seller Inventory # 9781461433071