Hit papers significantly outperform the citation benchmark for their cohort. A paper qualifies
if it has ≥500 total citations, achieves ≥1.5× the top-1% citation threshold for papers in the
same subfield and year (this is the minimum needed to enter the top 1%, not the average
within it), or reaches the top citation threshold in at least one of its specific research
topics.
Cosmic-Ray Heating of the Interstellar Gas
1969406 citationsG. B. Field, Donald Goldsmith et al.The Astrophysical Journalprofile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
hero ref
This map shows the geographic impact of H. J. Habing's research. It shows the number of citations coming from papers published by authors working in each country. You can also color the map by specialization and compare the number of citations received by H. J. Habing with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites H. J. Habing more than expected).
This network shows the impact of papers produced by H. J. Habing. Nodes represent research fields, and links connect fields that are likely to share authors. Colored nodes show fields that tend to cite the papers produced by H. J. Habing. The network helps show where H. J. Habing may publish in the future.
Co-authorship network of co-authors of H. J. Habing
This figure shows the co-authorship network connecting the top 25 collaborators of H. J. Habing.
A scholar is included among the top collaborators of H. J. Habing based on the total number of
citations received by their joint publications. Widths of edges
represent the number of papers authors have co-authored together.
Node borders
signify the number of papers an author published with H. J. Habing. H. J. Habing is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Cioni, Maria-Rosa L., H. J. Habing, C. Loup, N. Epchtein, & E. Deul. (2004). DENIS Results on the Magellanic Clouds. Msngr. 115. 22–26.1 indexed citations
Blommaert, J. A. D. L., et al.. (1993). Candidate oh ir stars in the outer parts of our galaxy. Leiden Repository (Leiden University). 267(1). 39–53.1 indexed citations
8.
Bliek, N. S. van der, P. Bouchet, H. J. Habing, et al.. (1992). Standard stars for the Infrared Space Observatory, ISO.. Open Repository and Bibliography (University of Liège).3 indexed citations
9.
Lindqvist, M., H. J. Habing, & A. Winnberg. (1992). OH/IR stars close to the Galactic Centre. II - Their spatial and kinematic properties and the mass distribution within 5-100 PC from the galactic centre. Leiden Repository (Leiden University). 259(1). 118–127.13 indexed citations
10.
Habing, H. J.. (1990). The Evolution of Red Giants to White Dwarfs - a Review of the Observational Evidence. 16.1 indexed citations
Habing, H. J., et al.. (1985). Time variations and shell sizes of OH masers in late-type stars. Leiden Repository (Leiden University). 59(3). 523–555.4 indexed citations
13.
Olnon, F. M., H. J. Habing, B. Baud, et al.. (1984). IRAS observations of OH/IR stars. The Astrophysical Journal. 278. L41–L41.32 indexed citations
14.
Habing, H. J., F. M. Olnon, A. Winnberg, H. E. Matthews, & B. Baud. (1983). OH/IR stars within one degree of the galactic centre. Leiden Repository (Leiden University). 128(1). 230–244.2 indexed citations
15.
Baud, B., H. J. Habing, H. E. Matthews, & A. Winnberg. (1979). A systematic search at 1612 MHz for OH maser sources. I - Survey near the Galactic Centre. Leiden Repository (Leiden University). 35. 179–192.
Field, G. B., Donald Goldsmith, & H. J. Habing. (1969). A Theoretical Model for the Interstellar Medium. Bulletin of the American Astronomical Society. 1. 240.3 indexed citations
18.
Habing, H. J.. (1968). The interstellar radiation density between 912 A and 2400 A. 19. 421.16 indexed citations
Habing, H. J.. (1966). High-velocity gas at intermediate latitudes and its relation to the outer part of the Galaxy. 18. 323.2 indexed citations
Rankless uses publication and citation data sourced from OpenAlex, an open and comprehensive
bibliographic database. While OpenAlex provides broad and valuable coverage of the global
research landscape, it—like all bibliographic datasets—has inherent limitations. These include
incomplete records, variations in author disambiguation, differences in journal indexing, and
delays in data updates. As a result, some metrics and network relationships displayed in
Rankless may not fully capture the entirety of a scholar's output or impact.