WFRF:(Caselli S.)
Sökning: WFRF:(Caselli S.) > The CHESS spectral ...
LIBRIS Formathandbok (Information om MARC21)
| Fältnamn | Indikatorer | Metadata |
|---|---|---|
| 000 | 05632naa a2201213 4500 | |
| 001 | oai:DiVA.org:su-51506 | |
| 003 | SwePub | |
| 008 | 110110s2010 | |||||||||||000 ||eng| | |
| 024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-515062 URI |
| 024 | 7 | a https://doi.org/10.1051/0004-6361/2010145822 DOI |
| 040 | a (SwePub)su | |
| 041 | a engb eng | |
| 042 | 9 SwePub | |
| 072 | 7 | a ref2 swepub-contenttype |
| 072 | 7 | a art2 swepub-publicationtype |
| 100 | 1 | a Codella, C.4 aut |
| 245 | 1 0 | a The CHESS spectral survey of star forming regions :b Peering into the protostellar shock L1157-B1. I. Shock chemical complexity |
| 264 | c 2010-07-16 | |
| 264 | 1 | b EDP Sciences,c 2010 |
| 338 | a print2 rdacarrier | |
| 500 | a authorCount :69 | |
| 520 | a We present the first results of the unbiased survey of the L1157-B1 bow shock, obtained with HIFI in the framework of the key program Chemical HErschel Survey of Star forming regions (CHESS). The L1157 outflow is driven by a low-mass Class 0 protostar and is considered the prototype of the so-called chemically active outflows. The bright blue-shifted bow shock B1 is the ideal laboratory for studying the link between the hot (~1000-2000 K) component traced by H2 IR-emission and the cold (~10-20 K) swept-up material. The main aim is to trace the warm gas chemically enriched by the passage of a shock and to infer the excitation conditions in L1157-B1. A total of 27 lines are identified in the 555-636 GHz region, down to an average 3σ level of 30 mK. The emission is dominated by CO(5-4) and H2O(110-101) transitions, as discussed by Lefloch et al. in this volume. Here we report on the identification of lines from NH3, H2CO, CH3OH, CS, HCN, and HCO+. The comparison between the profiles produced by molecules released from dust mantles (NH3, H2CO, CH3OH) and that of H2O is consistent with a scenario in which water is also formed in the gas-phase in high-temperature regions where sputtering or grain-grain collisions are not efficient. The high excitation range of the observed tracers allows us to infer, for the first time for these species, the existence of a warm (≥200 K) gas component coexisting in the B1 bow structure with the cold and hot gas detected from ground. Herschel is an ESA space observatory with science instruments provided by European-led principal Investigator consortia and with important participation from NASA.Table 1 is only available in electronic form at http://www.aanda.org | |
| 650 | 7 | a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe |
| 650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng |
| 653 | a ISM: individual objects: L1157 | |
| 653 | a ISM: molecules | |
| 653 | a stars: formation | |
| 653 | a Astronomy and astrophysics | |
| 653 | a Astronomi och astrofysik | |
| 653 | a Astronomy | |
| 653 | a astronomi | |
| 700 | 1 | a Lefloch, B.4 aut |
| 700 | 1 | a Ceccarelli, C.4 aut |
| 700 | 1 | a Cernicharo, J.4 aut |
| 700 | 1 | a Caux, E.4 aut |
| 700 | 1 | a Lorenzani, A.4 aut |
| 700 | 1 | a Viti, S.4 aut |
| 700 | 1 | a Hily-Blant, P.4 aut |
| 700 | 1 | a Parise, B.4 aut |
| 700 | 1 | a Maret, S.4 aut |
| 700 | 1 | a Nisini, B.4 aut |
| 700 | 1 | a Caselli, P.4 aut |
| 700 | 1 | a Cabrit, S.4 aut |
| 700 | 1 | a Pagani, L.4 aut |
| 700 | 1 | a Benedettini, M.4 aut |
| 700 | 1 | a Boogert, A.4 aut |
| 700 | 1 | a Gueth, F.4 aut |
| 700 | 1 | a Melnick, G.4 aut |
| 700 | 1 | a Neufeld, D.4 aut |
| 700 | 1 | a Pacheco, S.4 aut |
| 700 | 1 | a Salez, M.4 aut |
| 700 | 1 | a Schuster, K.4 aut |
| 700 | 1 | a Bacmann, A.4 aut |
| 700 | 1 | a Baudry, A.4 aut |
| 700 | 1 | a Bell, T.4 aut |
| 700 | 1 | a Bergin, E. A.4 aut |
| 700 | 1 | a Blake, G.4 aut |
| 700 | 1 | a Bottinelli, S.4 aut |
| 700 | 1 | a Castets, A.4 aut |
| 700 | 1 | a Comito, C.4 aut |
| 700 | 1 | a Coutens, A.4 aut |
| 700 | 1 | a Crimier, N.4 aut |
| 700 | 1 | a Dominik, C.4 aut |
| 700 | 1 | a Demyk, K.4 aut |
| 700 | 1 | a Encrenaz, P.4 aut |
| 700 | 1 | a Falgarone, E.4 aut |
| 700 | 1 | a Fuente, A.4 aut |
| 700 | 1 | a Gerin, M.4 aut |
| 700 | 1 | a Goldsmith, P.4 aut |
| 700 | 1 | a Helmich, F.4 aut |
| 700 | 1 | a Hennebelle, P.4 aut |
| 700 | 1 | a Henning, Th.4 aut |
| 700 | 1 | a Herbst, E.4 aut |
| 700 | 1 | a Jacq, T.4 aut |
| 700 | 1 | a Kahane, C.4 aut |
| 700 | 1 | a Kama, M.4 aut |
| 700 | 1 | a Klotz, A.4 aut |
| 700 | 1 | a Langer, W.4 aut |
| 700 | 1 | a Lis, D.4 aut |
| 700 | 1 | a Lord, S.4 aut |
| 700 | 1 | a Pearson, J.4 aut |
| 700 | 1 | a Phillips, T.4 aut |
| 700 | 1 | a Saraceno, P.4 aut |
| 700 | 1 | a Schilke, P.4 aut |
| 700 | 1 | a Tielens, X.4 aut |
| 700 | 1 | a van der Tak, F.4 aut |
| 700 | 1 | a van der Wiel, M.4 aut |
| 700 | 1 | a Vastel, C.4 aut |
| 700 | 1 | a Wakelam, V.4 aut |
| 700 | 1 | a Walters, A.4 aut |
| 700 | 1 | a Wyrowski, F.4 aut |
| 700 | 1 | a Yorke, H.4 aut |
| 700 | 1 | a Borys, C.4 aut |
| 700 | 1 | a Delorme, Y.4 aut |
| 700 | 1 | a Kramer, C.4 aut |
| 700 | 1 | a Larsson, Bengtu Stockholms universitet,Institutionen för astronomi4 aut0 (Swepub:su)bem |
| 700 | 1 | a Mehdi, I.4 aut |
| 700 | 1 | a Ossenkopf, V.4 aut |
| 700 | 1 | a Stutzki, J.4 aut |
| 710 | 2 | a Stockholms universitetb Institutionen för astronomi4 org |
| 773 | 0 | t Astronomy and Astrophysicsd : EDP Sciencesg 518, s. L112-q 518<L112-x 0004-6361x 1432-0746 |
| 856 | 4 | u https://www.aanda.org/articles/aa/pdf/2010/10/aa14582-10.pdf |
| 856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-51506 |
| 856 | 4 8 | u https://doi.org/10.1051/0004-6361/201014582 |
Hitta via bibliotek
- Astronomy and Astrophysics (Sök värdpublikationen i LIBRIS)
Till lärosätets databas
Hitta mer i SwePub
- Av författaren/redakt...
- Codella, C.
- Lefloch, B.
- Ceccarelli, C.
- Cernicharo, J.
- Caux, E.
- Lorenzani, A.
- visa fler...
- Viti, S.
- Hily-Blant, P.
- Parise, B.
- Maret, S.
- Nisini, B.
- Caselli, P.
- Cabrit, S.
- Pagani, L.
- Benedettini, M.
- Boogert, A.
- Gueth, F.
- Melnick, G.
- Neufeld, D.
- Pacheco, S.
- Salez, M.
- Schuster, K.
- Bacmann, A.
- Baudry, A.
- Bell, T.
- Bergin, E. A.
- Blake, G.
- Bottinelli, S.
- Castets, A.
- Comito, C.
- Coutens, A.
- Crimier, N.
- Dominik, C.
- Demyk, K.
- Encrenaz, P.
- Falgarone, E.
- Fuente, A.
- Gerin, M.
- Goldsmith, P.
- Helmich, F.
- Hennebelle, P.
- Henning, Th.
- Herbst, E.
- Jacq, T.
- Kahane, C.
- Kama, M.
- Klotz, A.
- Langer, W.
- Lis, D.
- Lord, S.
- Pearson, J.
- Phillips, T.
- Saraceno, P.
- Schilke, P.
- Tielens, X.
- van der Tak, F.
- van der Wiel, M.
- Vastel, C.
- Wakelam, V.
- Walters, A.
- Wyrowski, F.
- Yorke, H.
- Borys, C.
- Delorme, Y.
- Kramer, C.
- Larsson, Bengt
- Mehdi, I.
- Ossenkopf, V.
- Stutzki, J.
- visa färre...
- Om ämnet
-
- NATURVETENSKAP
- NATURVETENSKAP
- och Fysik
- och Astronomi astrof ...
- Artiklar i publikationen
- Astronomy and As ...
- Av lärosätet
- Stockholms universitet
Sök utanför SwePub
- Sök vidare i:
- Google Book Search
- Google Scholar
Kungliga biblioteket hanterar dina personuppgifter i enlighet med EU:s dataskyddsförordning (2018), GDPR. Läs mer om hur det funkar här.
Så här hanterar KB dina uppgifter vid användning av denna tjänst.
- Copyright © LIBRIS - Nationella bibliotekssystem
- LIBRIS.kb.se
