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How to maintain the star formation of the Milky Way Galaxy? On the value of single dish full-sky surveys Jrgen Kerp 1 , Benjamin Winkel 2 , Peter Kalberla 1 and the EBHIS team 1 Argelander-Institut fr Astronomie, Universitt Bonn 2


  1. „How to maintain the star formation of the Milky Way Galaxy?“ On the value of single dish full-sky surveys Jürgen Kerp 1 , Benjamin Winkel 2 , Peter Kalberla 1 and the EBHIS team 1 Argelander-Institut für Astronomie, Universität Bonn 2 Max-Planck-Institut für Radioastronomie jkerp@uni-bonn.de 1

  2. HI 21-cm line data Adopted Wikipedia jkerp@uni-bonn.de 2

  3. HI 21-cm line data Peak → lower limit to gas temperature FWHM → upper limit to gas temperature jkerp@uni-bonn.de 3

  4. Square Kilometer Array (SKA) Wikipedia jkerp@uni-bonn.de 4

  5. Single dish to radio interferometer jkerp@uni-bonn.de 5

  6. Single dish to radio interferometer jkerp@uni-bonn.de 6

  7. Single dish to radio interferometer jkerp@uni-bonn.de 7

  8. HVC 125+41-207: radio interferometer Braun & Burton 2000, A&A 354, 853 jkerp@uni-bonn.de 8

  9. HVC 125+41-207: Effelsberg dish Brüns, Kerp & Pagels 2001, A&A 370, L26 VII-9 jkerp@uni-bonn.de

  10. Radio interferometer are sensitive to small scale structure Single dish telescopes are sensitive to structures on scales of the observed area of interest jkerp@uni-bonn.de VII- 10

  11. Radio interferometer are sensitive to small scale structure Single dish telescopes are sensitive to structures on scales of the observed area of interest Single dish full-sky surveys can disclose structures across hundreds of square degrees jkerp@uni-bonn.de VII- 11

  12. Stray-radiation Winkel et al. (2016), A&A 585, 41 12

  13. Effelsberg-Bonn HI Survey (EBHIS) jkerp@uni-bonn.de 13

  14. Effelsberg-Bonn HI Survey (EBHIS) Effelsberg 100-m key-science project ● started in August 2008 ● first coverage finished spring 2013 ● angular resolution: 10.8’ ● velocity resolution: 1.4 km/s ● sensitivity: ~90 mK ● maximum redshift: 0.07 ● data are public (CDS) ● Motivated FPGA spectrometer technology! ● jkerp@uni-bonn.de 14

  15. Effelsberg-Bonn HI Survey (EBHIS) 10 TByte of raw data ● Software written from scratch ● Many new methods/algorithms developed ● – RFI mitigation (Flöer+ 2009) – Stray-radiation removal (Kalberla; see Winkel+ 2016a) – Flux calibration/Bandpass removal (Winkel & Kerp 2007; Winkel+ 2010, 2012a, 2016a) – Source finding/parametrization (Flöer & Winkel 2012; Flöer+ 1014) – Data gridding (Winkel+ 2016b) – Basket-weaving (Winkel+ 2012b) jkerp@uni-bonn.de 15

  16. jkerp@uni-bonn.de 16

  17. EBHIS first data release after two years jkerp@uni-bonn.de 17

  18. HI4PI: Effelsberg & Parkes Milky Way Surveys HI4PI collaboration: 2016 A&A 594, A116 jkerp@uni-bonn.de 18

  19. HI4PI still a top 10 paper of Astronomy & Astrophysics after a year jkerp@uni-bonn.de 19

  20. Kerp+ 2011 jkerp@uni-bonn.de Winkel+ 2016 20

  21. Kerp+ 2011 jkerp@uni-bonn.de Winkel+ 2016 21

  22. Kerp+ 2011 jkerp@uni-bonn.de Winkel+ 2016 22

  23. Green Bank Telescope: M31 HVCs Thilker, Braun & Westmeier 2005, ASP 331, 113 jkerp@uni-bonn.de 23

  24. EBHIS: M31 HVCs Kerp et al.. 2016, A&A 589, 120 jkerp@uni-bonn.de 24

  25. EBHIS: M31 HVCs Kerp et al.. 2016, A&A 589, 120 jkerp@uni-bonn.de 25

  26. „How to maintain the star formation of the Milky Way Galaxy?“ jkerp@uni-bonn.de 26

  27. Persistent fueling: no evidence for major mergers jkerp@uni-bonn.de 27

  28. Halo and disk-halo interface Marasco, Marinacci & Fraternali 2013, MNRAS 443, 1634 jkerp@uni-bonn.de 28

  29. Magnani & Smith 2010, ApJ 722, 1685 jkerp@uni-bonn.de 29

  30. Magnani & Smith 2010, ApJ 722, 1685 In 2010 about 11 molecular IVCs were known jkerp@uni-bonn.de 30

  31. jkerp@uni-bonn.de 31

  32. jkerp@uni-bonn.de 32

  33. Dust to HI gas molecular molecular atomic atomic T. Röhser 2016 Ph. D., U. Bonn jkerp@uni-bonn.de 33

  34. Finding molecular IVCs: Gaussian decomposition Kalberla & Haud 2015, A&A 578, A78 jkerp@uni-bonn.de 34

  35. IVC 86+38 T. Röhser 2016 Ph. D., U. Bonn jkerp@uni-bonn.de 35

  36. jkerp@uni-bonn.de 36

  37. jkerp@uni-bonn.de 37

  38. North Röhser et al. 2016, A&A 596, 94 jkerp@uni-bonn.de 38

  39. North HI 21-cm line data Röhser et al. 2016, A&A 596, 94 jkerp@uni-bonn.de 39

  40. South Röhser et al. 2016, A&A 596, 94 jkerp@uni-bonn.de 40

  41. South artefact MS Röhser et al. 2016, A&A 596, 94 jkerp@uni-bonn.de 41

  42. North-south asymmetry Total numbers of FIR excess IVCs ~ 1000!!!! 694 MIVCs towards the northern sky 389 toward the southern sky Large clouds (> 35 arcmin) Röhser et al. (2016), A&A 596, 94 jkerp@uni-bonn.de 42

  43. North-south asymmetry Total numbers of FIR excess IVCs 694 MIVCs towards the northern sky 389 toward the southern sky Large clouds (> 35 arcmin) Röhser et al. (2016), A&A 596, 94 jkerp@uni-bonn.de 43

  44. North-south asymmetry Total numbers of FIR excess IVCs 694 MIVCs towards the northern sky 389 toward the southern sky Large clouds (> 35 arcmin) Röhser et al. (2016), A&A 596, 94 jkerp@uni-bonn.de 44

  45. MIVCs: tiny extent and mass, but many Röhser et al. (2016), A&A 596, 94 jkerp@uni-bonn.de 45

  46. MIVCs: tiny extent and mass, but many Too faint and too tiny to detect them beyond the Magellanic Cloud System Röhser et al. (2016), A&A 596, 94 jkerp@uni-bonn.de 46

  47. MIVCs: tiny extent and mass, but many Total local mass of IVCs 3.1 10 6 M sun Up to 0.5 M sun a -1 Only 10% of the Milky Way halo is probed Röhser et al. (2016), A&A 596, 94 jkerp@uni-bonn.de 47

  48. What next? jkerp@uni-bonn.de 48

  49. EBHIS: confirmed galaxy detections Flöer 2015, PhD thesis Bonn University jkerp@uni-bonn.de 49

  50. EBHIS: Zone of avoidence Schöder, Flöer, Winkel in prep. jkerp@uni-bonn.de 50

  51. EBHIS: radio continuum full sky map Winkel et al., in prep. jkerp@uni-bonn.de 51

  52. Foregrounds jkerp@uni-bonn.de 52

  53. Polarization and Faraday rotation N HI map Planck polarization fraction Bachelor these A. Manthei 2017 jkerp@uni-bonn.de 53

  54. Polarization and Faraday rotation N HI map Planck Faraday rotation Bachelor these A. Manthei 2017 jkerp@uni-bonn.de 54

  55. Polarization and Faraday rotation Dust temperature (Planck) Faraday rotation Bachelor these A. Manthei 2017 jkerp@uni-bonn.de 55

  56. Cosmic infrared background (CIB) D. Lenz, 2016 Ph. D., U. Bonn jkerp@uni-bonn.de 56

  57. Cosmic infrared background (CIB) D. Lenz, 2016 Ph. D., U. Bonn jkerp@uni-bonn.de 57

  58. eRosita (2019): X-ray full-sky survey MPE jkerp@uni-bonn.de 58

  59. Dark Gas: correlation with X-rays HI 21-cm column density 0.25 keV ROSAT J. Kerp „X-ray astroomy“ 2003 jkerp@uni-bonn.de 59

  60. Thank you Poster of Charitarth Vyas on gas accretion jkerp@uni-bonn.de 60

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