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008			150903s2005 gw | o |||| 0|eng d
020			_a9783540316060 _99783540316060
024	7		_a10.1007/b96749 _2doi
035			_avtls000347821
039		9	_a201509030441 _bVLOAD _c201405070518 _dVLOAD _y201402070940 _zstaff
040			_aMX-SnUAN _bspa _cMX-SnUAN _erda
050		4	_aQB1-991
100	1		_aKäufl, Hans Ulrich. _eeditor. _9329581
245	1	0	_aHigh Resolution Infrared Spectroscopy in Astronomy : _bProceedings of an ESO Workshop Held at Garching, Germany, 18-21 November 2003 / _cedited by Hans Ulrich Käufl, Ralf Siebenmorgen, Alan F. M. Moorwood.
264		1	_aBerlin, Heidelberg : _bSpringer Berlin Heidelberg, _c2005.
300			_axx, 559 páginas Also available online. _brecurso en línea.
336			_atexto _btxt _2rdacontent
337			_acomputadora _bc _2rdamedia
338			_arecurso en línea _bcr _2rdacarrier
347			_aarchivo de texto _bPDF _2rda
490	0		_aESO Astrophysics Symposia, _x1431-2433
500			_aSpringer eBooks
505	0		_aInstrumentation and Observational Highlights -- Young Stars, Hot Stars, LBVs, Novae, SNe, ISM-1 -- Normal MS Stars, Old Stars, Active Stars, ISM-2 -- Solar Systems, Brown Dwarfs -- Our Solar System.
520			_aTwo specialized new instruments for ESO's VLT, VISIR and CRIRES, spawned the idea for this workshop. CRIRES is a dedicated very high resolution infrared spectrograph; VISIR features a high resolution spectroscopic mode. Together, the instruments combine the sensitivity of an 8m-telescope with the now well-established reliability of VLT-facility instruments. High resolution here means that lines in cool stellar atmospheres and HII-regions can be resolved. The astrophysical topics discussed in this rather specialized workshop range from the inner solar system to active galactic nuclei. There are many possibilities for new discoveries with these instruments, but the unique capability, which becomes available through high-resolution infrared spectroscopy, is the observation of molecular rotational-vibrational transitions in many astrophysical environments. Particularly interesting and surprising in this context, many papers on modeling and laboratory spectroscopy at the workshop appear to indicate that astronomical observations are lagging a bit behind in this field. The papers are an interesting mix of reports from existing high resolution facilities, reports on modeling efforts of synthetic spectra and reports on laboratory spectra. In this sense, a fruitful exchange between molecular physics and astronomy was again accomplished and is documented in this volume.
590			_aPara consulta fuera de la UANL se requiere clave de acceso remoto.
700	1		_aSiebenmorgen, Ralf. _eeditor. _9329582
700	1		_aMoorwood, Alan F. M. _eeditor. _9329583
710	2		_aSpringerLink (Servicio en línea) _9299170
776	0	8	_iEdición impresa: _z9783540252566
856	4	0	_uhttp://remoto.dgb.uanl.mx/login?url=http://dx.doi.org/10.1007/b96749 _zConectar a Springer E-Books (Para consulta externa se requiere previa autentificación en Biblioteca Digital UANL)
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