Atlas and Catalogue of Infrared Sources in the Magellanic Clouds:
Gespeichert in:
1. Verfasser: | |
---|---|
Format: | Elektronisch E-Book |
Sprache: | English |
Veröffentlicht: |
Dordrecht
Springer Netherlands
1990
|
Schlagworte: | |
Online-Zugang: | Volltext |
Beschreibung: | Around the beginning of the sixteenth century, Portuguese and Dutch sailors first ventured into southern seas. With their keen navigational interest in the skies, they noted the continuous presence of two cloud-like features, not far from the almost immediately Southern Pole. The first literature mention of these 'clouds' was in the journal written in 1520 by the Italian navigator Pigafetta on the first circumnavigation of the globe by Magalhaes (c/. Pigafetta et ai. , 1962). In honour of this exploit, the objects have since become known as the Magellanic Clouds, although the Dutch name 'Kaapsche Wolken' (Cape Clouds - after the Cape of Good Hope) has also been in use for centuries. The Large and Small Magellanic Clouds are dwarf irregular galaxies, orbiting our own Milky Way Galaxy, presently at distances of 53 and 63 kpc respectively (Humphreys, 1984) . . They are the galaxies nearest to us: most other Local Group galaxies are of order ten times more distant. The LMC and SMC are also the prototypical blue dwarf irregulars, representatives of a class of objects in which several hundred more distant objects are now known. Their masses are a few per cent of the mass of the Milky Way Galaxy, but they are relatively gas-rich and appear to be, at the present epoch, forming stars at a more prodiguous rate than our Galaxy (c/. Lequeux, 1984) |
Beschreibung: | 1 Online-Ressource (224p) |
ISBN: | 9789400905375 9789401067287 |
DOI: | 10.1007/978-94-009-0537-5 |
Internformat
MARC
LEADER | 00000nmm a2200000zc 4500 | ||
---|---|---|---|
001 | BV042414901 | ||
003 | DE-604 | ||
005 | 00000000000000.0 | ||
007 | cr|uuu---uuuuu | ||
008 | 150316s1990 |||| o||u| ||||||eng d | ||
020 | |a 9789400905375 |c Online |9 978-94-009-0537-5 | ||
020 | |a 9789401067287 |c Print |9 978-94-010-6728-7 | ||
024 | 7 | |a 10.1007/978-94-009-0537-5 |2 doi | |
035 | |a (OCoLC)863759170 | ||
035 | |a (DE-599)BVBBV042414901 | ||
040 | |a DE-604 |b ger |e aacr | ||
041 | 0 | |a eng | |
049 | |a DE-91 |a DE-83 | ||
082 | 0 | |a 520 |2 23 | |
084 | |a PHY 000 |2 stub | ||
100 | 1 | |a Schwering, P. B. W. |e Verfasser |4 aut | |
245 | 1 | 0 | |a Atlas and Catalogue of Infrared Sources in the Magellanic Clouds |c by P. B. W. Schwering, F. P. Israel |
264 | 1 | |a Dordrecht |b Springer Netherlands |c 1990 | |
300 | |a 1 Online-Ressource (224p) | ||
336 | |b txt |2 rdacontent | ||
337 | |b c |2 rdamedia | ||
338 | |b cr |2 rdacarrier | ||
500 | |a Around the beginning of the sixteenth century, Portuguese and Dutch sailors first ventured into southern seas. With their keen navigational interest in the skies, they noted the continuous presence of two cloud-like features, not far from the almost immediately Southern Pole. The first literature mention of these 'clouds' was in the journal written in 1520 by the Italian navigator Pigafetta on the first circumnavigation of the globe by Magalhaes (c/. Pigafetta et ai. , 1962). In honour of this exploit, the objects have since become known as the Magellanic Clouds, although the Dutch name 'Kaapsche Wolken' (Cape Clouds - after the Cape of Good Hope) has also been in use for centuries. The Large and Small Magellanic Clouds are dwarf irregular galaxies, orbiting our own Milky Way Galaxy, presently at distances of 53 and 63 kpc respectively (Humphreys, 1984) . . They are the galaxies nearest to us: most other Local Group galaxies are of order ten times more distant. The LMC and SMC are also the prototypical blue dwarf irregulars, representatives of a class of objects in which several hundred more distant objects are now known. Their masses are a few per cent of the mass of the Milky Way Galaxy, but they are relatively gas-rich and appear to be, at the present epoch, forming stars at a more prodiguous rate than our Galaxy (c/. Lequeux, 1984) | ||
650 | 4 | |a Physics | |
650 | 4 | |a Astronomy, Observations and Techniques | |
700 | 1 | |a Israel, F. P. |e Sonstige |4 oth | |
856 | 4 | 0 | |u https://doi.org/10.1007/978-94-009-0537-5 |x Verlag |3 Volltext |
912 | |a ZDB-2-PHA |a ZDB-2-BAE | ||
940 | 1 | |q ZDB-2-PHA_Archive | |
999 | |a oai:aleph.bib-bvb.de:BVB01-027850394 |
Datensatz im Suchindex
_version_ | 1804153081259098112 |
---|---|
any_adam_object | |
author | Schwering, P. B. W. |
author_facet | Schwering, P. B. W. |
author_role | aut |
author_sort | Schwering, P. B. W. |
author_variant | p b w s pbw pbws |
building | Verbundindex |
bvnumber | BV042414901 |
classification_tum | PHY 000 |
collection | ZDB-2-PHA ZDB-2-BAE |
ctrlnum | (OCoLC)863759170 (DE-599)BVBBV042414901 |
dewey-full | 520 |
dewey-hundreds | 500 - Natural sciences and mathematics |
dewey-ones | 520 - Astronomy and allied sciences |
dewey-raw | 520 |
dewey-search | 520 |
dewey-sort | 3520 |
dewey-tens | 520 - Astronomy and allied sciences |
discipline | Physik |
doi_str_mv | 10.1007/978-94-009-0537-5 |
format | Electronic eBook |
fullrecord | <?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>02602nmm a2200385zc 4500</leader><controlfield tag="001">BV042414901</controlfield><controlfield tag="003">DE-604</controlfield><controlfield tag="005">00000000000000.0</controlfield><controlfield tag="007">cr|uuu---uuuuu</controlfield><controlfield tag="008">150316s1990 |||| o||u| ||||||eng d</controlfield><datafield tag="020" ind1=" " ind2=" "><subfield code="a">9789400905375</subfield><subfield code="c">Online</subfield><subfield code="9">978-94-009-0537-5</subfield></datafield><datafield tag="020" ind1=" " ind2=" "><subfield code="a">9789401067287</subfield><subfield code="c">Print</subfield><subfield code="9">978-94-010-6728-7</subfield></datafield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/978-94-009-0537-5</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(OCoLC)863759170</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-599)BVBBV042414901</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-604</subfield><subfield code="b">ger</subfield><subfield code="e">aacr</subfield></datafield><datafield tag="041" ind1="0" ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="049" ind1=" " ind2=" "><subfield code="a">DE-91</subfield><subfield code="a">DE-83</subfield></datafield><datafield tag="082" ind1="0" ind2=" "><subfield code="a">520</subfield><subfield code="2">23</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">PHY 000</subfield><subfield code="2">stub</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Schwering, P. B. W.</subfield><subfield code="e">Verfasser</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Atlas and Catalogue of Infrared Sources in the Magellanic Clouds</subfield><subfield code="c">by P. B. W. Schwering, F. P. Israel</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="a">Dordrecht</subfield><subfield code="b">Springer Netherlands</subfield><subfield code="c">1990</subfield></datafield><datafield tag="300" ind1=" " ind2=" "><subfield code="a">1 Online-Ressource (224p)</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">Around the beginning of the sixteenth century, Portuguese and Dutch sailors first ventured into southern seas. With their keen navigational interest in the skies, they noted the continuous presence of two cloud-like features, not far from the almost immediately Southern Pole. The first literature mention of these 'clouds' was in the journal written in 1520 by the Italian navigator Pigafetta on the first circumnavigation of the globe by Magalhaes (c/. Pigafetta et ai. , 1962). In honour of this exploit, the objects have since become known as the Magellanic Clouds, although the Dutch name 'Kaapsche Wolken' (Cape Clouds - after the Cape of Good Hope) has also been in use for centuries. The Large and Small Magellanic Clouds are dwarf irregular galaxies, orbiting our own Milky Way Galaxy, presently at distances of 53 and 63 kpc respectively (Humphreys, 1984) . . They are the galaxies nearest to us: most other Local Group galaxies are of order ten times more distant. The LMC and SMC are also the prototypical blue dwarf irregulars, representatives of a class of objects in which several hundred more distant objects are now known. Their masses are a few per cent of the mass of the Milky Way Galaxy, but they are relatively gas-rich and appear to be, at the present epoch, forming stars at a more prodiguous rate than our Galaxy (c/. Lequeux, 1984)</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Physics</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Astronomy, Observations and Techniques</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Israel, F. P.</subfield><subfield code="e">Sonstige</subfield><subfield code="4">oth</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">https://doi.org/10.1007/978-94-009-0537-5</subfield><subfield code="x">Verlag</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">ZDB-2-PHA</subfield><subfield code="a">ZDB-2-BAE</subfield></datafield><datafield tag="940" ind1="1" ind2=" "><subfield code="q">ZDB-2-PHA_Archive</subfield></datafield><datafield tag="999" ind1=" " ind2=" "><subfield code="a">oai:aleph.bib-bvb.de:BVB01-027850394</subfield></datafield></record></collection> |
id | DE-604.BV042414901 |
illustrated | Not Illustrated |
indexdate | 2024-07-10T01:20:56Z |
institution | BVB |
isbn | 9789400905375 9789401067287 |
language | English |
oai_aleph_id | oai:aleph.bib-bvb.de:BVB01-027850394 |
oclc_num | 863759170 |
open_access_boolean | |
owner | DE-91 DE-BY-TUM DE-83 |
owner_facet | DE-91 DE-BY-TUM DE-83 |
physical | 1 Online-Ressource (224p) |
psigel | ZDB-2-PHA ZDB-2-BAE ZDB-2-PHA_Archive |
publishDate | 1990 |
publishDateSearch | 1990 |
publishDateSort | 1990 |
publisher | Springer Netherlands |
record_format | marc |
spelling | Schwering, P. B. W. Verfasser aut Atlas and Catalogue of Infrared Sources in the Magellanic Clouds by P. B. W. Schwering, F. P. Israel Dordrecht Springer Netherlands 1990 1 Online-Ressource (224p) txt rdacontent c rdamedia cr rdacarrier Around the beginning of the sixteenth century, Portuguese and Dutch sailors first ventured into southern seas. With their keen navigational interest in the skies, they noted the continuous presence of two cloud-like features, not far from the almost immediately Southern Pole. The first literature mention of these 'clouds' was in the journal written in 1520 by the Italian navigator Pigafetta on the first circumnavigation of the globe by Magalhaes (c/. Pigafetta et ai. , 1962). In honour of this exploit, the objects have since become known as the Magellanic Clouds, although the Dutch name 'Kaapsche Wolken' (Cape Clouds - after the Cape of Good Hope) has also been in use for centuries. The Large and Small Magellanic Clouds are dwarf irregular galaxies, orbiting our own Milky Way Galaxy, presently at distances of 53 and 63 kpc respectively (Humphreys, 1984) . . They are the galaxies nearest to us: most other Local Group galaxies are of order ten times more distant. The LMC and SMC are also the prototypical blue dwarf irregulars, representatives of a class of objects in which several hundred more distant objects are now known. Their masses are a few per cent of the mass of the Milky Way Galaxy, but they are relatively gas-rich and appear to be, at the present epoch, forming stars at a more prodiguous rate than our Galaxy (c/. Lequeux, 1984) Physics Astronomy, Observations and Techniques Israel, F. P. Sonstige oth https://doi.org/10.1007/978-94-009-0537-5 Verlag Volltext |
spellingShingle | Schwering, P. B. W. Atlas and Catalogue of Infrared Sources in the Magellanic Clouds Physics Astronomy, Observations and Techniques |
title | Atlas and Catalogue of Infrared Sources in the Magellanic Clouds |
title_auth | Atlas and Catalogue of Infrared Sources in the Magellanic Clouds |
title_exact_search | Atlas and Catalogue of Infrared Sources in the Magellanic Clouds |
title_full | Atlas and Catalogue of Infrared Sources in the Magellanic Clouds by P. B. W. Schwering, F. P. Israel |
title_fullStr | Atlas and Catalogue of Infrared Sources in the Magellanic Clouds by P. B. W. Schwering, F. P. Israel |
title_full_unstemmed | Atlas and Catalogue of Infrared Sources in the Magellanic Clouds by P. B. W. Schwering, F. P. Israel |
title_short | Atlas and Catalogue of Infrared Sources in the Magellanic Clouds |
title_sort | atlas and catalogue of infrared sources in the magellanic clouds |
topic | Physics Astronomy, Observations and Techniques |
topic_facet | Physics Astronomy, Observations and Techniques |
url | https://doi.org/10.1007/978-94-009-0537-5 |
work_keys_str_mv | AT schweringpbw atlasandcatalogueofinfraredsourcesinthemagellanicclouds AT israelfp atlasandcatalogueofinfraredsourcesinthemagellanicclouds |