The Way Forward
Abstract For the last few decades the study of disks around stars young and old and of different types have progressed significantly. During the same time a completely new discipline—the study of exoplanets, planets orbiting stars other than our Sun—have emerged. Both these fields, which are interco...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Fridlund, Malcolm [verfasserIn] |
|---|
| Format: |
Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
2016 |
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| Schlagwörter: |
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| Anmerkung: |
© The Author(s) 2016 |
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| Übergeordnetes Werk: |
Enthalten in: Space science reviews - Springer Netherlands, 1962, 205(2016), 1-4 vom: 12. Mai, Seite 349-372 |
|---|---|
| Übergeordnetes Werk: |
volume:205 ; year:2016 ; number:1-4 ; day:12 ; month:05 ; pages:349-372 |
| Links: |
|---|
| DOI / URN: |
10.1007/s11214-016-0247-2 |
|---|
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OLC2033702731 |
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| 520 | |a Abstract For the last few decades the study of disks around stars young and old and of different types have progressed significantly. During the same time a completely new discipline—the study of exoplanets, planets orbiting stars other than our Sun—have emerged. Both these fields, which are interconnected, have benefited from the development of new instrumentation, and especially by telescopes and detectors deployed in space. In this chapter we are describing the state of the art of such instruments and make an inventory of what is being currently developed. We also state some of the requirements of the next steps and what type of instruments will lead the way forward. | ||
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Abstract For the last few decades the study of disks around stars young and old and of different types have progressed significantly. During the same time a completely new discipline—the study of exoplanets, planets orbiting stars other than our Sun—have emerged. Both these fields, which are interconnected, have benefited from the development of new instrumentation, and especially by telescopes and detectors deployed in space. In this chapter we are describing the state of the art of such instruments and make an inventory of what is being currently developed. We also state some of the requirements of the next steps and what type of instruments will lead the way forward. © The Author(s) 2016 |
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Abstract For the last few decades the study of disks around stars young and old and of different types have progressed significantly. During the same time a completely new discipline—the study of exoplanets, planets orbiting stars other than our Sun—have emerged. Both these fields, which are interconnected, have benefited from the development of new instrumentation, and especially by telescopes and detectors deployed in space. In this chapter we are describing the state of the art of such instruments and make an inventory of what is being currently developed. We also state some of the requirements of the next steps and what type of instruments will lead the way forward. © The Author(s) 2016 |
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Abstract For the last few decades the study of disks around stars young and old and of different types have progressed significantly. During the same time a completely new discipline—the study of exoplanets, planets orbiting stars other than our Sun—have emerged. Both these fields, which are interconnected, have benefited from the development of new instrumentation, and especially by telescopes and detectors deployed in space. In this chapter we are describing the state of the art of such instruments and make an inventory of what is being currently developed. We also state some of the requirements of the next steps and what type of instruments will lead the way forward. © The Author(s) 2016 |
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<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">OLC2033702731</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230504050845.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">200819s2016 xx ||||| 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/s11214-016-0247-2</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC2033702731</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-He213)s11214-016-0247-2-p</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">600</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">16,12</subfield><subfield code="2">ssgn</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Fridlund, Malcolm</subfield><subfield code="e">verfasserin</subfield><subfield code="0">(orcid)0000-0002-0855-8426</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">The Way Forward</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2016</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">ohne Hilfsmittel zu benutzen</subfield><subfield code="b">n</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Band</subfield><subfield code="b">nc</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">© The Author(s) 2016</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract For the last few decades the study of disks around stars young and old and of different types have progressed significantly. 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