1987
DOI: 10.1086/165648
|View full text |Cite
|
Sign up to set email alerts
|

Solar system-sized condensations in the Orion Nebula

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
4
1

Citation Types

11
180
1

Year Published

2003
2003
2024
2024

Publication Types

Select...
4
2
1

Relationship

0
7

Authors

Journals

citations
Cited by 186 publications
(192 citation statements)
references
References 0 publications
11
180
1
Order By: Relevance
“…Evidence suggests that the proplyds are undergoing mass loss from photoevaporation by the nearby O star q 1 Ori C, so the free-free emission we detect here is likely due to a wind (e.g., Churchwell et al 1987;Henney & Arthur 1998). For emission from a spherically symmetric wind with an arbitrary µ a -n r density profile the expected spectral dependence of free-free emission is (Wright & Barlow 1975).…”
Section: Estimating the Free-free Emission Spectrummentioning
confidence: 68%
See 3 more Smart Citations
“…Evidence suggests that the proplyds are undergoing mass loss from photoevaporation by the nearby O star q 1 Ori C, so the free-free emission we detect here is likely due to a wind (e.g., Churchwell et al 1987;Henney & Arthur 1998). For emission from a spherically symmetric wind with an arbitrary µ a -n r density profile the expected spectral dependence of free-free emission is (Wright & Barlow 1975).…”
Section: Estimating the Free-free Emission Spectrummentioning
confidence: 68%
“…They were first identified as free-free emission by Garay et al (1987), and suggested to be the ionized material evaporated from protostellar disks by Churchwell et al (1987). Observations of the ONC with the HST firmly established these compact structures as externally ionized protoplanetary disks (e.g., O'Dell et al 1993).…”
Section: Introductionmentioning
confidence: 99%
See 2 more Smart Citations
“…Together they cover an area of a few square arcminutes. This area is also one of the most crowded with YSOs emitting at radio frequencies (i.e., Churchwell et al 1987;Garay et al 1987;Zapata et al 2004;Kounkel et al 2014;Forbrich et al 2016). Taking advantage of these characteristics and using multi-epoch observations, the proper motion of several objects were measured by Gómez et al (2005Gómez et al ( , 2008.…”
Section: Introductionmentioning
confidence: 99%