An International Workshop on
Interstellar Matter and Star Formation
- A Multi-Wavelength Perspective
(A Part of the Homi Bhabha Birth Centenary Celebrations)
October 5 - 7, 2009
Venue : TIFR NATIONAL BALLOON FACILITY, HYDERABAD, INDIA
Scientific Objectives
Star formation is one of the most important areas of research in astrophysics.
Observationally, our method of investigating the star formation process has
changed in the last 4 - 5 years. Recent advances in infrared and
(sub) millimeter detector technology has resulted in new wide field
cameras that allow mapping of large areas of the sky in reasonable observation times. With the
advancement in technology, new challenging observations will be able
to answer some of the unresolved issues regarding modes of star and planet
formation. The current and new facilities such as WFCAM on UKIRT, UKIDSS, ESO-VISTA
(infrared), SCUBA2, HARP, 4MASS (radio) on the ground and the space missions such as
AKARI, Spitzer Space Telescope, Herschel (to be launched in mid 2009) and Planck
will provide a great depth and coverage in multiple wavelengths. On the other hand, the
upcoming facilities such as ALMA in the millimeter wavelengths and the JWST in the
infrared will provide angular resolution at milli-arcsecond levels to probe distant
objects at AU scales. SPICA in the mid-/far-infrared, to be launched in 2017, will
fill the gap in the coverage of wavelength between JWST and Herschel.
With these upcoming facilities it will be possible to observe a
significant area of star forming regions in a short time scale. Consequently, this will
provide a chance to address the central issues in star formation studies. The all
sky samples covering large fraction of the sky will provide an opportunity to
carry out unbiased statistical studies of young stellar properties, the
distribution of sub-stellar objects, the structure of molecular clouds, initial mass
function and mechanism of massive star formation.
The purpose of the workshop is to expose and motivate students and young researchers
towards this field and to promote the topic of Star Formation at the graduate
studies level so that the upcoming young generation in India can efficiently use
the next generation space and ground based telescope facilities such as
Herschel, JWST, ALMA, VISTA and SCUBA/JCMT. The workshop will also focus
on results from the currently operational state-of-art ground based near- and
mid-infrared and sub-mm and millimeter observatories.
The year 2009 also marks completion of 25 years of the TIFR 100 cm balloon borne infrared
telescope and this workshop would also commemorate the occasion.
Science Topics
B. G. Anandarao (India) W. P. Chen (Taiwan) D. Froebrich (UK) G. Fuller (UK) S. K. Ghosh (India) M. Gopinath (India) H. Kaneda (Japan) M. W. Knight (UK) B. Mookerjea (India) T. Nakagawa (Japan) Y. Nakajima (Japan) M. S. Nanda Kumar (Portugal) K. Ogura (Japan) D. K. Ojha (India) T. Onaka (Japan) A. K. Pandey (India) T. P. Prabhu (India) A. N. Ramprakash (India) R. Sagar (India) I. Sakon (Japan) S. Schmeja (Germany) M. Tamura (Japan) S. N. Tandon (India) P. S. Teixeira (Germany) ......
Scientific Organizing Committee
N. M. Ashok (PRL, India) H. C. Bhatt (IIA, India) S. K. Ghosh (TIFR, India) B. Mookerjea (TIFR, India) T. Nakagawa (ISAS-JAXA, Japan) M. S. Nanda Kumar (CAUP, Portugal) D. K. Ojha (Chair, TIFR, India) A. K. Pandey (ARIES, India) T. P. Prabhu (IIA, India) A. N. Ramprakash (IUCAA, India) R. Sagar (ARIES, India) M. D. Smith (CAPS, UK) M. Tamura (NAOJ, Japan)
Local Organizing Committee
S. L. D’Costa (Secretary) (TIFR, Mumbai) S. K. Ghosh (TIFR, Mumbai) R. K. Manchanda (TIFR, Mumbai) B. Mookerjea (TIFR, Mumbai) D. K. Ojha (Chair) (TIFR, Mumbai) L. Singh (TIFR NBF, Hyderabad) S. Sreenivasan (Co-Chair) (TIFR NBF, Hyderabad) J. V. Subbarao (TIFR NBF, Hyderabad) B. Suneel Kumar (TIFR NBF, Hyderabad)
Location
TIFR Balloon Facility is located about 17 km from Hyderabad city and is next to the ECIL campus. Hyderabad is well connected to the rest of the world by both national and international flights. The airport is called Rajiv Gandhi International Airport and is located at Shamshabad.
Registered Participants
1. Anandarao B.G. (PRL, Ahmedabad) 2. Bhatt B.C. (IIA, Bangalore) 3. Bhatt H.C. (IIA, Bangalore) 4. Borgaonkar S.S. (TIFR, Mumbai) 5. Chakraborti Sayan (TIFR, Mumbai) 6. Chauhan Neelam (ARIES, Nainital) 7. Chen Wen Ping (National Central University, Taiwan) 8. Choudhury Rumpa (IIA, Bangalore) 9. Das Mousumi (BITS, Hyderabad) 10. Dewangan Lokesh (PRL, Ahmedabad) 11. Eswaraiah C. (ARIES, Nainital) 12. Froebrich Dirk (University of Kent, UK) 13. Fuller Gary (University of Manchester, UK) 14. Ghosh Swarna K. (TIFR, Mumbai) 15. Hasan Priya (Osmania University, Hyderabad) 16. Jerin Paul K. (TIFR, Mumbai) 17. Jose Jessy (ARIES, Nainital) 18. Joshi U.C. (PRL, Ahmedabad) 19. Kaneda Hidehiro (Nagoya University, Japan) 20. Kaurav S.S. (TIFR, Mumbai) 21. Knight M.W. (University of Kent, UK) 22. Lakhchaura Kiran (TIFR, Mumbai) 23. Maheswar Gopinathan (ARIES, Nainital) 24. Manchanda Ravi (TIFR, Mumbai) 25. Mathew Blesson (IIA, Bangalore) 26. Mookerjea B. (TIFR, Mumbai) 27. Nakajima Yasushi (Nagoya University/NAOJ, Japan) 28. Nakagawa Takao (ISAS/JAXA, Japan) 29. Nanda Kumar M.S. (CAUP, Porto, Portugal) 30. Ogura Katsuo (Kokugakuin University, Japan) 31. Ojha Devendra (TIFR, Mumbai) 32. Onaka Takashi (University of Tokyo, Japan) 33. Pandey A.K. (ARIES, Nainital) 34. Pandey S.K. (Pt Ravishankar Shukla University, Raipur) 35. Pawade V.S. (Mumbai Univ., Mumbai) 36. Prabhu T.P. (IIA, Bangalore) 37. Ramaprakash A.N. (IUCAA, Pune) 38. Rao P. Vivekananda (Osmania University, Hyderabad) 39. Rengarajan T.N. (Mumbai) 40. Roy Subhashis (NCRA-TIFR, Pune) 41. Sagar Ram (ARIES, Nainital) 42. Sahu D.K. (IIA, Bangalore) 43. Sakon Itsuki (University of Tokyo, Japan) 44. Samal Manash Ranjan (ARIES, Nainital, India) 45. Schmeja Stefan (Heidelberg University, Germany) 46. Shaw Gargi (TIFR, Mumbai) 47. Shimonishi Takashi (University of Tokyo, Japan) 48. Subramaniam Annapurni (IIA, Bangalore) 49. Tamura Motohide (NAOJ, Japan) 50. Tandon Shyam (IUCAA, Pune) 51. Tej Anandmayee (IIST, Thiruvananthpuram) 52. Teixeira Paula Stella (European Southern Observatory, Germany) 53. Todmal S.S. (TIFR, Mumbai) 54. Vaidya D.B. (Gujarat Arts and Science College, Ahmedabad) 55. Verma R.P. (Mumbai) 56. Vig Sarita (IIT, Chennai) 57. Yadav R.K. (ARIES, Nainital)
Other Participants
1. Bakalkar C. B. (TIFR, Mumbai) 2. D'Costa S. L. (TIFR, Mumbai) 3. Jadhav R. B. (TIFR, Mumbai) 4. Kumar Suneel B. (BF, TIFR) 5. Meshram G. S. (TIFR, Mumbai) 6. Naik M. B. (TIFR, Mumbai) 7. Poojary S. S. (TIFR, Mumbai) 8. Sandimani P. (TIFR, Mumbai) 9. Singh L. (BF, TIFR) 10. Sreenivasan S. (BF, TIFR) 11. Subbarao J. V. (BF, TIFR)
Scientific Programme
Please click here for Scientific Programme. Please NOTE: The Scientific Programme may undergo some changes depending on the availability of the speaker.Abstracts
Please click here for the abstracts of the talks.Poster Abstracts
The space available for each poster is 90 cm x 110 cm (width x height), which can fit A1 size posters. Please click here to see the poster abstracts.
PROCEEDINGS of the Workshop
All the presentations at the Interstellar Matter and Star Formation - A Multi-Wavelength Perspective workshop will be published after a refereeing process in a special issue of the Bulletin of the Astronomical Society of India. The Proceedings Volume will be made available online on the BASI webpage, as well as on ADS. We would be pleased if all the speakers could submit their proceedings articles at the time of the workshop. A LaTeX2e class file (basi.cls) is available for preparing your manuscript in the BASI format. For users of LaTeX2.09, style file basi.sty is also available. Further details can be found at http://www.ncra.tifr.res.in/~basi/instructions.htm. The following Page limits apply: Invited review (30 + 5 = 35 min): 8 pages
Invited contributed talk (25 + 5 = 30 min / 20 + 5 = 25 min): 6 pages
Contributed talk (15 + 5 = 20 min): 4 pages
Poster paper: 2 pages
Tourism
Hyderabad is the capital city of Andhra Pradesh and the fifth largest city of India. In addition to its historical significance, Hyderabad is one of the major IT hubs of India, housing more than 150 major IT companies. Hyderabad is known for its rich history, culture and architecture, and also known as The City of Nizams and The City of Pearls. The 13th century Golconda Fort is one of the most wonderful monuments, located 11 km from Hyderabad.
For those workshop participants who are interested in tourism, many city tours around Hyderabad are organized by the Hyderabad Tourism Department.