Details on Acronym: [CMH2010] | |
| [CMH2010] | (Cormier+Madden+Hony+, 2010) (Not yet in Simbad) |
| Write: | <<[CMH2010] NGC 4214-R>> |
| N: | 3 |
| Object: | MCld (SIMBAD class: MolCld = Molecular Cloud) |
| Note: | Herschel PACS spectroscopic maps of the dwarf galaxy NGC 4214. Use of CO(1-0) contours from Walter et al. 2001AJ....121..727W. Regions NGC 4214-I and -II are centered on the [C II] peaks, while region NGC 4214-III was chosen by taking into account the peak of the CO emission. |
| in source: | NGC 4214 |
| Ref: | =2010A&A...518L..57C |
| by | CORMIER D. , MADDEN S.C., HONY S., CONTURSI A., POGLITSCH A., GALLIANO F., STURM E., DOUBLIER V., FEUCHTGRUBER H., GALAMETZ M., GEIS N., DE JONG J., OKUMURA K., PANUZZO P., SAUVAGE M. |
| Astron. Astrophys., 518L, 57-57 (2010) | |
| The effects of star formation on the low-metallicity ISM: NGC 4214 mapped with Herschel/PACS spectroscopy. | |
| o | Fig. 2, Table 1: <[CMH2010] NGC 4214-R> (Nos I-III). |