Extended CO(3-2) emission in our targets. The first two columns show the IRAS PSC identification and alternative names for our targets. The third column lists the FWHM determined by fitting a Gaussian to the radial profile of the velocity-integrated line intensity, while the fourth column shows the full extent of that quantity in the form of the diameter where the emission equals 3σ, averaged ringwise. Where no value is given this measurement could not be made, and instead we evaluate whether extended emission is marginal (?) or not detected (N) in the preliminary JCMT CO(3-2) maps. Sources marked with * are also in the DEATHSTAR sample.
| IRAS PSC # . | simbad ID . | FWHM (arcsec) . | Extent (arcsec) . |
|---|---|---|---|
| IRAS 00205+5530 | T Cas | 15.2 | 27 |
| IRAS 01556+4511 | V370 And | 15.6 | 33 |
| IRAS 03507+1115 | IK Tau | 19.2 | 57 |
| IRAS 04020-1551 | V Eri | 17.4 | N |
| IRAS 04566+5606 | TX Cam | 15.3 | 39 |
| IRAS 07120-4433 | L2 Pup* | 21.4 | 33 |
| IRAS 08003+3629 | SV Lyn | 18.1 | N |
| IRAS 09448+1139 | R Leo* | 21.6 | 51 |
| IRAS 09452+1330 | IRC+10216 | 43.9 | 222 |
| IRAS 10329-3918 | U Ant | 40.8 | 63 |
| IRAS 11461-3542 | V919 Cen | 15.7 | ? |
| IRAS 12277+0441 | BK Vir* | 14.2 | N |
| IRAS 13001+0527 | RT Vir* | 19.0 | 33 |
| IRAS 13114-0232 | SW Vir* | 18.4 | 51 |
| IRAS 13368-4941 | V744 Cen | 13.4 | ? |
| IRAS 13462-2807 | W Hya* | 18.3 | 45 |
| IRAS 15492+4837 | ST Her | 18.8 | 27 |
| IRAS 16235+1900 | U Her | 20.2 | ? |
| IRAS 18359+0847 | X Oph | 15.0 | N |
| IRAS 19039+0809 | R Aql | 16.0 | 39 |
| IRAS 19126-0708 | W Aql | 18.0 | 63 |
| IRAS 21088+6817 | T Cep | 18.1 | 27 |
| IRAS 21439-0226 | EP Aqr | 15.6 | 45 |
| IRAS 22196-4612 | π1 Gru | 23.3 | 51 |
| IRAS 23320+4316 | LP And | 18.2 | 63 |
| IRAS PSC # . | simbad ID . | FWHM (arcsec) . | Extent (arcsec) . |
|---|---|---|---|
| IRAS 00205+5530 | T Cas | 15.2 | 27 |
| IRAS 01556+4511 | V370 And | 15.6 | 33 |
| IRAS 03507+1115 | IK Tau | 19.2 | 57 |
| IRAS 04020-1551 | V Eri | 17.4 | N |
| IRAS 04566+5606 | TX Cam | 15.3 | 39 |
| IRAS 07120-4433 | L2 Pup* | 21.4 | 33 |
| IRAS 08003+3629 | SV Lyn | 18.1 | N |
| IRAS 09448+1139 | R Leo* | 21.6 | 51 |
| IRAS 09452+1330 | IRC+10216 | 43.9 | 222 |
| IRAS 10329-3918 | U Ant | 40.8 | 63 |
| IRAS 11461-3542 | V919 Cen | 15.7 | ? |
| IRAS 12277+0441 | BK Vir* | 14.2 | N |
| IRAS 13001+0527 | RT Vir* | 19.0 | 33 |
| IRAS 13114-0232 | SW Vir* | 18.4 | 51 |
| IRAS 13368-4941 | V744 Cen | 13.4 | ? |
| IRAS 13462-2807 | W Hya* | 18.3 | 45 |
| IRAS 15492+4837 | ST Her | 18.8 | 27 |
| IRAS 16235+1900 | U Her | 20.2 | ? |
| IRAS 18359+0847 | X Oph | 15.0 | N |
| IRAS 19039+0809 | R Aql | 16.0 | 39 |
| IRAS 19126-0708 | W Aql | 18.0 | 63 |
| IRAS 21088+6817 | T Cep | 18.1 | 27 |
| IRAS 21439-0226 | EP Aqr | 15.6 | 45 |
| IRAS 22196-4612 | π1 Gru | 23.3 | 51 |
| IRAS 23320+4316 | LP And | 18.2 | 63 |
Extended CO(3-2) emission in our targets. The first two columns show the IRAS PSC identification and alternative names for our targets. The third column lists the FWHM determined by fitting a Gaussian to the radial profile of the velocity-integrated line intensity, while the fourth column shows the full extent of that quantity in the form of the diameter where the emission equals 3σ, averaged ringwise. Where no value is given this measurement could not be made, and instead we evaluate whether extended emission is marginal (?) or not detected (N) in the preliminary JCMT CO(3-2) maps. Sources marked with * are also in the DEATHSTAR sample.
| IRAS PSC # . | simbad ID . | FWHM (arcsec) . | Extent (arcsec) . |
|---|---|---|---|
| IRAS 00205+5530 | T Cas | 15.2 | 27 |
| IRAS 01556+4511 | V370 And | 15.6 | 33 |
| IRAS 03507+1115 | IK Tau | 19.2 | 57 |
| IRAS 04020-1551 | V Eri | 17.4 | N |
| IRAS 04566+5606 | TX Cam | 15.3 | 39 |
| IRAS 07120-4433 | L2 Pup* | 21.4 | 33 |
| IRAS 08003+3629 | SV Lyn | 18.1 | N |
| IRAS 09448+1139 | R Leo* | 21.6 | 51 |
| IRAS 09452+1330 | IRC+10216 | 43.9 | 222 |
| IRAS 10329-3918 | U Ant | 40.8 | 63 |
| IRAS 11461-3542 | V919 Cen | 15.7 | ? |
| IRAS 12277+0441 | BK Vir* | 14.2 | N |
| IRAS 13001+0527 | RT Vir* | 19.0 | 33 |
| IRAS 13114-0232 | SW Vir* | 18.4 | 51 |
| IRAS 13368-4941 | V744 Cen | 13.4 | ? |
| IRAS 13462-2807 | W Hya* | 18.3 | 45 |
| IRAS 15492+4837 | ST Her | 18.8 | 27 |
| IRAS 16235+1900 | U Her | 20.2 | ? |
| IRAS 18359+0847 | X Oph | 15.0 | N |
| IRAS 19039+0809 | R Aql | 16.0 | 39 |
| IRAS 19126-0708 | W Aql | 18.0 | 63 |
| IRAS 21088+6817 | T Cep | 18.1 | 27 |
| IRAS 21439-0226 | EP Aqr | 15.6 | 45 |
| IRAS 22196-4612 | π1 Gru | 23.3 | 51 |
| IRAS 23320+4316 | LP And | 18.2 | 63 |
| IRAS PSC # . | simbad ID . | FWHM (arcsec) . | Extent (arcsec) . |
|---|---|---|---|
| IRAS 00205+5530 | T Cas | 15.2 | 27 |
| IRAS 01556+4511 | V370 And | 15.6 | 33 |
| IRAS 03507+1115 | IK Tau | 19.2 | 57 |
| IRAS 04020-1551 | V Eri | 17.4 | N |
| IRAS 04566+5606 | TX Cam | 15.3 | 39 |
| IRAS 07120-4433 | L2 Pup* | 21.4 | 33 |
| IRAS 08003+3629 | SV Lyn | 18.1 | N |
| IRAS 09448+1139 | R Leo* | 21.6 | 51 |
| IRAS 09452+1330 | IRC+10216 | 43.9 | 222 |
| IRAS 10329-3918 | U Ant | 40.8 | 63 |
| IRAS 11461-3542 | V919 Cen | 15.7 | ? |
| IRAS 12277+0441 | BK Vir* | 14.2 | N |
| IRAS 13001+0527 | RT Vir* | 19.0 | 33 |
| IRAS 13114-0232 | SW Vir* | 18.4 | 51 |
| IRAS 13368-4941 | V744 Cen | 13.4 | ? |
| IRAS 13462-2807 | W Hya* | 18.3 | 45 |
| IRAS 15492+4837 | ST Her | 18.8 | 27 |
| IRAS 16235+1900 | U Her | 20.2 | ? |
| IRAS 18359+0847 | X Oph | 15.0 | N |
| IRAS 19039+0809 | R Aql | 16.0 | 39 |
| IRAS 19126-0708 | W Aql | 18.0 | 63 |
| IRAS 21088+6817 | T Cep | 18.1 | 27 |
| IRAS 21439-0226 | EP Aqr | 15.6 | 45 |
| IRAS 22196-4612 | π1 Gru | 23.3 | 51 |
| IRAS 23320+4316 | LP And | 18.2 | 63 |
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