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Stanke, Thomas - European Southern Observatory (ESO)
An unbiased infrared H 2 for embedded flows
3 Observations In the following section I will describe the various data that were used to search for the outflows and
jets and molecular (CO) outflows: Details A number of molecular (CO) outflows are known in the survey area. Here I will compare the H 2 data to existing
7 Discussion 7.1 Jet & protostar statistics in Orion A
Astronomy & Astrophysics manuscript no. July 12, 2002 (DOI: will be inserted by hand later)
An unbiased infrared H 2 for embedded flows
An unbiased infrared H 2 for embedded flows
In this chapter, the properties of the jet sample will be presented in detail. The focus will be on the properties of the sample as such, not so much on properties of individual objects. This keeps with
Molecular CO outflows in the L1641N cluster: kneading a cloud T. Stanke 1,2
Astronomy & Astrophysics manuscript no. 1331 November 1, 2005 (DOI: will be inserted by hand later)
C The outflow driving sources In this section I present a list of candidate driving sources for the outlows listed.
In this section a compilation of all H 2 emission line features is presented. Figure 13 gives an overview over the entire survey area, with the areas covered by the 9 individual survey fields indicated. In the
In this section a list of outflows identified from the H 2 survey is given. First, I give for each field an overview, with the candidate outflows regarded as rather certain
168 A THE H 2 A.7 Field 7
Jets and CS cores Tatematsu et al. (1993; T93 in the following) performed a CS (1--0) survey of a large part of the Orion A
8 Conclusions and future prospects 8.1 Conclusions
2 Star formation and outflows: an overview 2.1 The current picture of lowmass star formation
1 Flows from young stellar objects 1.1 The need for an unbiased survey
4 Data analysis 4.1 The nearinfrared H 2 survey
Astronomy & Astrophysics manuscript no. (will be inserted by hand later)
A.4 Field 4 151 A.4 Field 4
