Purple Mountain Observatory Workshop: Star Formation and ISM in Starforming Galaxies Near and Far----中国科学院紫金山天文台

Seminar Title	Purple Mountain Observatory Workshop: Star Formation and ISM in Starforming Galaxies Near and Far

	DAY 1, Sunday Sept. 20 Section 1: Distant SF/ISM 9:00 am – 9:35 am Greve, T. (UCL) ‘Galaxy wanderings’ 9:35 am – 10: 05 am Huang, J. (NAOC) MIPS 24um selected ULIRGs at z~2: the largest sample! 30 10:05 am – 10:35 am Fan, L. (SDU) ‘Extreme starburst in hyper-luminous hot dust-obscured galaxies at z~3’ 30 10:35 am – 11:00 am Coffee/Tea Break 11:00 am – 11:30 am Shu, X. (AHNU) ‘On the z~>4 dusty SF galaxies selected with Herschel’ 30 11:30 am -12:00 am Hao, C. (TJNU) ‘Lyman-alpha emitting galaxies at z~2.23’ 12:00 pm – 12: 30 pm 1st FOCUS DISCUSSION: the ALMA era & Group Photo Lunch 12:30–2pm AFTERNOON Section 2: Nearby SF/ISM: Star Formation Law 2: 00 pm – 2:30 pm Shi, Y. (NJU) Roles of existing stars in star formation 2:30 pm – 3:00 pm Zhu, M. (NAOC) ‘HI and star formation’ 3:00 pm – 3:30 pm Wang, J. (SHAO) ‘Isotopic lines of dense gas tracers in galaxies’ 3:30 pm – 4: 00 pm Coffee/Tea Break 4:00 pm – 4:30 pm Gao, Yu (PMO) 'Star formation law in galaxies' 4:30 pm- 5:00 pm Xiao, T. (SHAO) 'CO gas observations of MaNGA galaxies’ 5:00 pm – 5:30 pm Shi, S. (PMO) “Terahertz superconducting imaging array & other developments” 5:30 pm – 6:00 pm 2nd FOCUS DISCUSSION: THz/Dome-A 6:00 pm Workshop Dinner DAY 2, Monday Sept. 21 Section 3: Nearby SF/ISM: SF/AGN &Feedback 9:00 am – 9:30 am Hao, L. (SHAO) ‘Dust and AGN’ 9:30 am – 10:00 am Chen, X (SHAO) ‘Class I methanol megamaser - a new probe of starburst activity and feedback in active galaxies’ 30 10:00 am – 10:30 am Chen, Y. (NJU) ‘Galaxies with misalign gas and star kinematics from MaNGA’ 30 10: 30 am – 11:00 am Coffee/Tea Break 11:00 am – 11:30 am Romeo, A. (PMO)“3D Simulations of AGN jet feedback” 11: 30 am – 12:00 am Li, Z. (NJU) ‘The Galactic center and/or nearby edge-on galaxies in the scope of SF-ISM Interaction' 12:00 pm – 12:30 pm 3rd FOCUS DISCUSSION: Feedback 30 12:30 pm – 2:00 pm Lunch AFTERNOON Section 4: Nearby SF/ISM: Extreme systems & MaNGA 2:00 pm – 2:20 pm Tan, Q. (PMO) ‘Ultraluminous Infrared QSOs’ 2:20 pm – 2:40 pm Sethuram, R. (SHAO) ' Evolving Perspectives on Low Surface Brightness galaxies using MaNGA’ 2:40 pm – 2:55 pm Liu, W. (SHAO) ' Kpc-scale outflows in MaNGA galaxies' 2:55 pm – 3:10 pm Gao, Yang (SHAO) ‘CO observations of MaNGA galaxies carried out at PMO/Delingha’ 3:10 pm – 3:25 pm Zhou, L. (NJU) ‘The spatially resolved dust properties of metal poor galaxies’ 3:25 pm -3:40 pm Jin, Y. (NJU) ‘The global properties of counter-rotating disks’ 3:40 pm – 4: 10 pm Coffee/Tea Break 4:10 pm – 4:30 pm Jin, Z. (PMO) ‘Macronova in GRB 060614: evidence for the merger of a neutron star-black hole binary system)’ Any other talks and short contributions Afternoon Discussion: Dinner

Organisers:	Hongjun Ma (PMO), Yu Gao (PMO), Thomas Greve (UCL)

When：	Sep. 20-21

Venue:	Room 517 , Office Block, 2 West Beijing Road (PMO, CAS)

	Welcome to Attend

	( PMO Academic Committee & Academic Circulating committee)

Abstract　　　

We are fortunate to be astronomers in an era where a number of truly groundbreaking facilities — from ALMA, JWST, to SKA — are becoming available. The implications are that we could be only decades from a comprehensive understanding of galaxy formation and evolution and its complex interplay with star formation and the ISM. Obviously, this will require interdisciplinarity between such diverse areas as star formation, astro-chemistry and ISM physics to cosmic structure growth, active galactic nuclei and outflow physics. And this interplay will have to be mapped out from the epoch of reionization to the present day. No small task…. !

This workshop will bring together researchers (from students to senior staff) within a number of fields relevant to the overarching theme of the workshop. Example questions could range from

1) What is the role of mergers in galaxy evolution vs. secular evolution, and what is the imprint on the ISM and star formation properties of the galaxies?

2) How do outflows shape the lives of galaxies?

3) How do we best infer the distributions of gas density and mass in the ISM of galaxies?

4) How do we probe the deeply embedded nuclei of IR-luminous galaxies where extreme dust-obscuration hides the central power source?

The above are merely examples questions, and by no means exhaustive. The aim of the workshop is to create an informal atmosphere rich in discussion, questions, (crazy) ideas, and suggestions for possible future directions.