Class information for: |
Basic class information |
Class id | #P | Avg. number of references |
Database coverage of references |
---|---|---|---|
6429 | 1484 | 37.5 | 59% |
Hierarchy of classes |
The table includes all classes above and classes immediately below the current class. |
Cluster id | Level | Cluster label | #P |
---|---|---|---|
19 | 4 | ASTRONOMY & ASTROPHYSICS//ASTROPHYSICAL JOURNAL//ASTRON | 523489 |
19 | 3 | ASTRONOMY & ASTROPHYSICS//ASTROPHYSICAL JOURNAL//ASTRON | 118981 |
38 | 2 | STARS FORMATION//ISM CLOUDS//ISM MOLECULES | 31753 |
6429 | 1 | ISM INDIVIDUAL ORION NEBULA//ISM INDIVIDUAL OBJECTS ORION NEBULA//H II REGIONS | 1484 |
Terms with highest relevance score |
rank | Term | termType | Chi square | Shr. of publ. in class containing term |
Class's shr. of term's tot. occurrences |
#P with term in class |
---|---|---|---|---|---|---|
1 | ISM INDIVIDUAL ORION NEBULA | authKW | 1097442 | 5% | 68% | 79 |
2 | ISM INDIVIDUAL OBJECTS ORION NEBULA | authKW | 193166 | 1% | 72% | 13 |
3 | H II REGIONS | authKW | 191752 | 10% | 6% | 153 |
4 | ISM MOLECULES | authKW | 166275 | 15% | 4% | 225 |
5 | ISM INDIVIDUAL NGC 2024 | authKW | 165963 | 1% | 73% | 11 |
6 | INFRARED ISM LINES AND BANDS | authKW | 153220 | 4% | 13% | 57 |
7 | ISM INDIVIDUAL ORION IRC2 | authKW | 151501 | 1% | 82% | 9 |
8 | ISM INDIVIDUAL OBJECTS NGC 2024 | authKW | 126018 | 0% | 88% | 7 |
9 | ISM INDIVIDUAL ORION | authKW | 119887 | 1% | 45% | 13 |
10 | ISM INDIVIDUAL OBJECTS OMC1 | authKW | 119703 | 1% | 73% | 8 |
Web of Science journal categories |
Rank | Term | Chi square | Shr. of publ. in class containing term |
Class's shr. of term's tot. occurrences |
#P with term in class |
---|---|---|---|---|---|
1 | Astronomy & Astrophysics | 80998 | 95% | 0% | 1412 |
2 | Optics | 33 | 4% | 0% | 52 |
3 | Engineering, Aerospace | 2 | 0% | 0% | 6 |
4 | Instruments & Instrumentation | -1 | 1% | 0% | 11 |
5 | Spectroscopy | -1 | 0% | 0% | 7 |
6 | Meteorology & Atmospheric Sciences | -2 | 0% | 0% | 7 |
7 | Multidisciplinary Sciences | -2 | 0% | 0% | 1 |
8 | Geosciences, Multidisciplinary | -6 | 1% | 0% | 8 |
9 | Physics, Fluids & Plasmas | -7 | 0% | 0% | 1 |
10 | Physics, Applied | -7 | 2% | 0% | 34 |
Address terms |
Rank | Term | Chi square | Shr. of publ. in class containing term |
Class's shr. of term's tot. occurrences |
#P with term in class |
---|---|---|---|---|---|
1 | RADIOASTRON ASTROFIS | 38598 | 2% | 6% | 32 |
2 | 900 LEILANI ST | 20575 | 0% | 100% | 1 |
3 | ABT MUNCHBERG | 20575 | 0% | 100% | 1 |
4 | ASTRON PROGRAM EARTH ENVIRONM SCI | 20575 | 0% | 100% | 1 |
5 | ASTRON SONDERFOR BEREICH RADIOASTRON 131 | 20575 | 0% | 100% | 1 |
6 | ASTRON SONDERSFOR BEREICH RADIOASTRON 131 | 20575 | 0% | 100% | 1 |
7 | ASTROPHYS MEGURO KU | 20575 | 0% | 100% | 1 |
8 | ASTROPHYS OPT PHYS | 20575 | 0% | 100% | 1 |
9 | CEADSMCNRS AIM | 20575 | 0% | 100% | 1 |
10 | CNRSUMR 8112OBSERV PARIS | 20575 | 0% | 100% | 1 |
Journals |
Rank | Term | Chi square | Shr. of publ. in class containing term |
Class's shr. of term's tot. occurrences |
#P with term in class |
---|---|---|---|---|---|
1 | ASTROPHYSICAL JOURNAL | 92916 | 40% | 1% | 594 |
2 | ASTRONOMY & ASTROPHYSICS | 22559 | 16% | 0% | 236 |
3 | IAU SYMPOSIA | 10270 | 4% | 1% | 63 |
4 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 9685 | 10% | 0% | 145 |
5 | ASTRONOMICAL JOURNAL | 7381 | 5% | 1% | 72 |
6 | ASTRONOMY LETTERS-A JOURNAL OF ASTRONOMY AND SPACE ASTROPHYSICS | 6976 | 2% | 1% | 28 |
7 | REVISTA MEXICANA DE ASTRONOMIA Y ASTROFISICA | 5272 | 1% | 1% | 18 |
8 | ASTROPHYSICS AND SPACE SCIENCE | 3987 | 3% | 0% | 50 |
9 | INFRARED PHYSICS | 3888 | 1% | 1% | 14 |
10 | PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC | 2604 | 2% | 0% | 26 |
Author Key Words |
Core articles |
The table includes core articles in the class. The following variables is taken into account for the relevance score of an article in a cluster c: (1) Number of references referring to publications in the class. (2) Share of total number of active references referring to publications in the class. (3) Age of the article. New articles get higher score than old articles. (4) Citation rate, normalized to year. |
Rank | Reference | # ref. in cl. |
Shr. of ref. in cl. |
Citations |
---|---|---|---|---|
1 | VAN DER WERF, PP , GOSS, WM , O'DELL, CR , (2013) TEARING THE VEIL: INTERACTION OF THE ORION NEBULA WITH ITS NEUTRAL ENVIRONMENT.ASTROPHYSICAL JOURNAL. VOL. 762. ISSUE 2. P. - | 79 | 79% | 12 |
2 | O'DELL, CR , FERLAND, GJ , HENNEY, WJ , PEIMBERT, M , GARCIA-DIAZ, MT , RUBIN, RH , (2015) THE NATURE AND FREQUENCY OF OUTFLOWS FROM STARS IN THE CENTRAL ORION NEBULA CLUSTER.ASTRONOMICAL JOURNAL. VOL. 150. ISSUE 4. P. - | 78 | 74% | 1 |
3 | GENZEL, R , STUTZKI, J , (1989) THE ORION MOLECULAR CLOUD AND STAR-FORMING REGION.ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS. VOL. 27. ISSUE . P. 41 -85 | 104 | 62% | 399 |
4 | NISSEN, HD , CUNNINGHAM, NJ , GUSTAFSSON, M , BALLY, J , LEMAIRE, JL , FAVRE, C , FIELD, D , (2012) A 3D VIEW OF THE OUTFLOW IN THE ORION MOLECULAR CLOUD 1 (OMC-1).ASTRONOMY & ASTROPHYSICS. VOL. 540. ISSUE . P. - | 51 | 77% | 13 |
5 | O'DELL, CR , HENNEY, WJ , ABEL, NP , FERLAND, GJ , ARTHUR, SJ , (2009) THE THREE-DIMENSIONAL DYNAMIC STRUCTURE OF THE INNER ORION NEBULA.ASTRONOMICAL JOURNAL. VOL. 137. ISSUE 1. P. 367 -382 | 62 | 68% | 20 |
6 | O'DELL, CR , (2001) THE ORION NEBULA AND ITS ASSOCIATED POPULATION.ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS. VOL. 39. ISSUE . P. 99 -136 | 82 | 55% | 156 |
7 | HOLLENBACH, DJ , TIELENS, AGGM , (1999) PHOTODISSOCIATION REGIONS IN THE INTERSTELLAR MEDIUM OF GALAXIES.REVIEWS OF MODERN PHYSICS. VOL. 71. ISSUE 1. P. 173 -230 | 126 | 30% | 342 |
8 | TIELENS, AGGM , HOLLENBACH, DJ , (1997) DENSE PHOTODISSOCIATION REGIONS (PDRS).ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS. VOL. 35. ISSUE . P. 179 -215 | 88 | 43% | 296 |
9 | HIROTA, T , KIM, MK , KURONO, Y , HONMA, M , (2015) ALMA IMAGING OF MILLIMETER/SUBMILLIMETER CONTINUUM EMISSION IN ORION KL.ASTROPHYSICAL JOURNAL. VOL. 801. ISSUE 2. P. - | 37 | 80% | 3 |
10 | HIROTA, T , KIM, MK , HONMA, M , (2016) ALMA OBSERVATION OF THE 658 GHZ VIBRATIONALLY EXCITED H2O MASER IN ORION KL SOURCE I.ASTROPHYSICAL JOURNAL. VOL. 817. ISSUE 2. P. - | 37 | 71% | 1 |
Classes with closest relation at Level 1 |